This galaxy presents as a fairly smooth, elliptical-like structure. The light distribution is centrally concentrated, with a bright core that fades gradually into the outer regions. There is a slight elongation, giving it a somewhat flattened appearance.

The color profile suggests a relatively old stellar population, with a dominant yellow-orange hue. There is little evidence of significant dust lanes or prominent spiral arm features. Subtle irregularities or disturbances hint at potential tidal interactions or past merger events. A faint, diffuse halo surrounds the central region, suggesting a spheroidal distribution of stars.