The galaxy presents as a largely featureless, elliptical morphology. The overall color profile is predominantly yellow-orange, suggesting a stellar population that is largely composed of older stars. There is minimal evidence of spiral arm structures or significant dust lanes, supporting the classification as an elliptical galaxy. The light is concentrated towards the center, with a smooth, gradual decrease in luminosity outwards. The shape is primarily rounded, but appears to be slightly oblong. There is no visible indication of any recent or ongoing major mergers or tidal disturbances.
