The galaxy appears to be a relatively compact, elliptical galaxy. Its light profile suggests a smooth, centrally concentrated luminosity distribution, indicative of an older stellar population. The galaxy exhibits a generally round morphology and minimal apparent disk-like structure. It has a prominent core with decreasing luminosity towards its outer edges. No apparent active galactic nucleus or prominent dust lanes are visible. The color indices suggest the galaxy consists predominantly of older stars. There is no evidence of ongoing mergers or tidal disturbances.
