The galaxy presents a generally smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with the brightest region located at the core. The galaxy displays a slight elongation, deviating marginally from a perfect circular shape. The color gradient suggests a possible redder core region with bluer regions towards the outer edges. There are no discernable spiral arm structures or prominent dust lanes. The overall appearance indicates a relatively evolved system, likely with a significant population of older stars. There may be some signs of minor disturbances but the galaxy shows little evidence of any major merging activity or tidal features.
