The galaxy presents as an elliptical morphology, characterized by a centrally concentrated luminosity profile that diminishes gradually outwards. The core exhibits a distinct yellowish-white hue, indicative of a population dominated by older stars. This central region appears relatively smooth and lacks discernible substructure. Extending outward from the core, a less intense halo of reddish-orange light is observed. This outer halo is more diffuse, and suggests the presence of a slightly younger stellar population than that of the core. There is no apparent spiral arm structure or dust lane features, reinforcing the classification as an elliptical type galaxy. The overall shape appears nearly circular on the plane of the sky. No strong signs of tidal disturbances or ongoing mergers are apparent.
