The article points out, "One problem in forming such a system is that gas giants are thought to take 5 to 10 million years to accrete all their gas from the planet-forming disk around them. However, the current models suggest that such a disk in a binary system survives for less than 1 million years before gravitational tides from the companion star break the disk apart. Furthermore, in the case of GJ 896AB, the two stars are red dwarfs, which makes the existence of a gas giant planet in the system even more surprising. Scientists think red dwarfs lack the necessary amount of raw material to form giant planets, but the presence of a gas giant in this binary system suggests that planets could form differently when there are two stars present. "Additional detailed studies of this and similar systems can help us gain important insights into how planets are formed in binary systems," Sanchez-Bermudez said."
I read about this system at phys.org. First full 3D view of binary star-planet system from VLBA,
https://phys.org/news/2022-09-full-3d-view-binary-star-planet.html
My observation. The phys.org report calls attention to how difficult it is to explain the origin of this exoplanet around the binary star system using the protoplanetary disc model. "In particular, current models indicate that such a large planet is very unlikely as a companion to such a small star, so maybe those models need to be adjusted," he added. The astrometric technique will be a valuable tool for characterizing more planetary systems, the astronomers said.”
Ref - 3D Orbital Architecture of a Dwarf Binary System and Its Planetary Companion,
https://iopscience.iop.org/article/10.3847/1538-3881/ac7c66, 01-Sep-2022. “Abstract Because of the diversity of stellar masses and orbital sizes of binary systems and the complex interaction between star–star, star–planet, and planet–planet, it has been difficult to fully characterize the planetary systems associated with binary systems. Here, we report high-precision astrometric observations of the low-mass binary system GJ 896AB, revealing the presence of a Jupiter-like planetary companion (GJ 896Ab). The planetary companion is associated to the main star GJ 896A, with an estimated mass of 2.3 Jupiter masses and an orbit period of 284.4 days..."
The Extrasolar Planet Encyclopaedia — GJ 896A b (exoplanet.eu), the value for e is large too, 0.35.