Surely the edges of galaxies are fuzzy, then thinning about exponentially. Perhaps the half way point between galaxies occasionally has a millionth the mass of the average mass within 100 light years of our solar system. More is likely typical.
Objects and particles traveling away (approximately) from the center of a galaxy typically keep going for at least 100 light years before they fall back into the galaxy like cannon shell at the top of it's trajectory. The 200 light years travel outside the galaxy could last a billion years, but somewhat less is likely typical. Outside for a million times a million years is likely extremely rare and has not happened yet as the Universe is only 13.7 billion years old. Like planets, galaxies do sweep up some of the mass that they collide with as they travel. Most galaxies do travel and are typically orbiting the other galaxies in their local group of galaxies. We think the local groups are traveling in random directions vectorially added to the expansion of the Universe, which is why rare galactic groups show blue shift rather than red shift.
Photons and neutrinos, are only slowed very slightly by the average gravity of a galaxy, so they may average 1% of the number typical in our Oort cloud. What is lacking almost entirely is stars that have ten or more times the absolute luminosity of our sun, as most of these become compact stars, before they leave the galaxy.
Are there other mechanisms besides sling shot maneuvers at work to get mass between the galaxies? Neil