The galaxy presents as a fairly smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing quite round in projection. There is no prominent disk structure or spiral arm features discernable. The core region is relatively bright and concentrated, surrounded by a fainter, more diffuse halo. Color gradients suggest a population of older stars, as indicated by the yellowish-red hue, particularly within the galaxy's core. There is an apparent lack of significant dust lanes or prominent star-forming regions. Based on its morphology and color, the galaxy is likely an early-type galaxy, possibly an elliptical galaxy, at a considerable distance. A potential tidal disturbance or minor merging event cannot be ruled out, although no major disturbances are readily apparent.
