  We present the results of N-body simulations of dissipationless galaxy
merging in Modified Newtonian Dynamics (MOND). For comparison, we also studied
Newtonian merging between galaxies embedded in dark matter halos, with internal
dynamics equivalent to the MOND systems. We found that the merging timescales
are significantly longer in MOND than in Newtonian gravity with dark matter,
suggesting that observational evidence of rapid merging could be difficult to
explain in MOND. However, when two galaxies eventually merge, the MOND merging
end-product is hardly distinguishable from the final stellar distribution of an
equivalent Newtonian merger with dark matter.
