Okay, interesting, perhaps a flat planet too
The paper states, "6. Conclusions
Disc-instability protoplanets are not spherically symmetric, but close to being oblate spheroids. Their outer regions show more complex, asymmetric structure due to interactions with the protostellar disc and their formation history. Gas accretion happens faster from the protoplanet poles than from the protoplanet equator. We expect that this may lead to a strong modification of the observed properties of protoplanets (e.g. their spectrum, Hα emission; see Zhu 2015; Marleau et al. 2022, 2023) with the viewing angle that needs to be taken into account when interpreting observations, like those of PDS 70 b,c (Keppler et al.
2018; Haffert et al. 2019) and AB Aurigae b (Currie et al. 2022)."
PDS 70 system is confirmed,
https://exoplanet.eu/catalog/pds_70_b--6770/
Detailed information about planet PDS 70 c and its parameters.
exoplanet.eu
https://exoplanet.eu/catalog/ab_aur_b--522/, is a confirmed exoplanet too. How giant impacts during planet formation in various disc masses could alter their shapes too I did not see disclosed.