The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The light profile suggests a lack of significant spiral arm structure. It has a generally round morphology. The color index, based on visual inspection, suggests a population of older stars with less active star formation, consistent with a more evolved system. There may be some minor disturbance to the upper edge of the halo, but most likely not a major event. The galaxy's overall appearance indicates it is not actively merging with another system and exhibits minimal signs of tidal disruption.
