From the Wikipedia article [0] on NGC 1052:
NGC 1052 shows also two small jets emerging from its
nucleus as well as a very extended disc of neutral
hydrogen, far larger than the galaxy itself,
all these features suggesting a gas-rich galaxy
collided and merged with it 1 billion years ago
producing all the above features.
Is it possible that NGC 1052-DF2 is simply the remnant of the aforementioned gas-rich galaxy suspected of having collided with NGC 1052, and that the apparent dark matter deficiency is a result of that collision?Or do we know what happens when galaxies collide well enough to conclude with reasonable certainty that this is not the case?