The galaxy presents as a largely featureless elliptical or lenticular system. It exhibits a smooth, centrally concentrated light distribution, with a high degree of circularity. There is little to no evidence of spiral arms or a prominent disk structure. The galaxy possesses a bright central bulge that gradually fades outward. The overall color appears to be somewhat blue-white, suggesting the presence of some younger stellar populations. No significant dust lanes or signs of active star formation are readily apparent in the image. A slight asymmetry in the outer isophotes may indicate a minor gravitational interaction or past merger event, but it is subtle. The galaxy appears relatively undisturbed overall.
