The galaxy appears to be relatively compact with a bright, concentrated central region that exhibits a bluish-white color, indicative of hotter, younger stars and/or an active galactic nucleus. The inner core is surrounded by a more diffuse halo. 

There are several distinct and seemingly detached regions of varying color. There is some evidence for what could be minor disturbances or tidal features. The overall shape deviates from a pure elliptical form, possibly due to an ongoing or recent interaction/merger, or complex internal processes. 
