The galaxy presents as a largely smooth object with a somewhat elliptical morphology. There appears to be minimal evidence of spiral arm structure or prominent dust lanes. The color profile suggests an older stellar population, trending towards redder wavelengths across the observed light. Light is concentrated in the core and falls off fairly smoothly. This is consistent with an early-type galaxy, either an elliptical or lenticular type. There are no strong indications of ongoing major merging events, although some minor asymmetry in the outer regions may suggest past or ongoing interactions. The general appearance indicates a relatively evolved system.
