The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge, with a gradual decrease in luminosity towards its outer regions. There is little evidence of spiral arms or significant dust lanes. The galaxy appears somewhat spheroidal, with a minor axis ratio suggestive of a slightly flattened shape. The color gradient indicates a population of older stars, with a yellowish hue dominating the galactic body, particularly towards the center. There are some indications of it being a high-Sersic index galaxy. There does not appear to be significant recent star formation activity.
