Pegasus I is located at 50 Mpc and is dominated by two massive
elliptical galaxies: NGC 7619 and NGC 7626. This group, though
not very massive, is rich in late-type galaxies and represents an
interesting environment to study several phenomena related to galaxy
evolution (interactions, fusions, harrassment, etc.): the fusion of two
sub-groups seem to be taking place. In this context we began the study
of the globular clusters associated to the two dominant galaxies, and
the dwarf galaxies that are found around them. Our aim is to try to
identify the physical processes involved in the assembling of Pegasus I.