The galaxy presents as a centrally concentrated, luminous spheroid with a smooth, amorphous structure.  Its core is a bright yellowish-white, indicative of a population of older stars.  The color suggests a relatively quiescent galaxy with little ongoing star formation in the core.  There are two minor reddish regions that do not appear to have spiral structure, and could be either areas of slightly more recent star formation, or dust. There are no obvious signs of a spiral arm structure or a well-defined disk. There may be some evidence of tidal disruption, but it could also be an artifact. 
