The galaxy presents as a relatively smooth, centrally concentrated elliptical. There is very little discernible disk structure. The object appears quite round, with no obvious tidal features or major disturbances indicative of a recent major merger. A subtle color gradient is observable, shifting from a slightly bluer hue in the outer regions to a redder central core. Based on the overall color profile, the galaxy likely has a population of older stars, and very little current star formation.
