The galaxy presents as a fairly compact, elliptical-like structure with a smooth appearance. The color profile suggests a population dominated by older stars, exhibiting a reddish-yellow hue. There is little discernible internal structure or spiral arm morphology evident. The galaxy appears well-defined, with no obvious signs of major tidal disturbances or ongoing mergers. The overall round shape is apparent. There appears to be only a slight possibility of a minor merging event or tidal disruption.
