The galaxy presents as a centrally concentrated, elliptical morphology. The light profile exhibits a smooth gradient, with the highest luminosity concentrated towards the nucleus. There is no discernible disk component, spiral arm structure, or prominent dust lanes. The galaxy appears slightly elongated, with an intermediate ellipticity. Its color is generally yellowish-white, suggesting a stellar population dominated by older stars and a relatively low rate of ongoing star formation. The galaxy appears relatively undisturbed, showing no significant tidal features or signs of a major merger event. There may be a slight asymmetry or minor perturbation in the outer regions, indicating a possible minor interaction. Overall, the galaxy appears to be a relatively massive early-type galaxy at a considerable distance.
