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The bright galaxy population of the Local Group Analog (LGA) LGG 225 has beenimaged with the Galaxy Evolution Explorer (GALEX) through its Far- and Near-UVwavebands. A significant fraction of the group members appear to underwentrecent/on-going interaction episodes that strongly disturbed overall galaxymorphology. UV-bright regions, sites of intense star formation activityaccompanied by intense dust extinction, mark the galaxy outskirts formingirregular structures and tails. Compared to the Local Group, LGG 225 seems thusto be experiencing a more intense and active evolutionary phase.

The impact of encounters on the members of Local Group Analogs. A view from GALEX