  The bright galaxy population of the Local Group Analog (LGA) LGG 225 has been
imaged with the Galaxy Evolution Explorer (GALEX) through its Far- and Near-UV
wavebands. A significant fraction of the group members appear to underwent
recent/on-going interaction episodes that strongly disturbed overall galaxy
morphology. UV-bright regions, sites of intense star formation activity
accompanied by intense dust extinction, mark the galaxy outskirts forming
irregular structures and tails. Compared to the Local Group, LGG 225 seems thus
to be experiencing a more intense and active evolutionary phase.
