The galaxy presents as a largely smooth, elliptical-type morphology. It exhibits a concentrated central bulge region with a gradual decrease in luminosity outward. The galaxy shows a color gradient, with the core appearing more yellow-orange, potentially indicating an older stellar population. There are slight hints of bluer regions on the periphery, suggestive of some level of recent star formation, although these are not sharply defined spiral arm features. There may be a minor asymmetry to the outer isophotes, potentially indicative of a past minor merger or interaction. The overall structure lacks prominent features such as dust lanes or spiral arms, indicating it is primarily comprised of older stars.
