The galaxy presents as a relatively smooth, centrally concentrated structure with a discernible elliptical morphology. The central region exhibits a bright, yellowish hue, suggesting a significant population of older stars. There is some extension in the horizontal direction with some faint possible features, implying a slight deviation from a perfect spheroid. The lack of readily apparent spiral arms or dust lanes indicates a classification toward the elliptical or lenticular galaxy types. The galaxy's color profile suggests an evolved stellar population and subdued current star formation. There's no obvious presence of strong tidal features indicating recent major mergers.
