The galaxy presents as an elliptical or lenticular system, with a smooth, centrally concentrated light distribution. The core region exhibits a strong luminosity, transitioning into a fainter, diffuse halo that extends along a major axis. The galaxy's shape is more elongated than circular. There is a suggestion of subtle asymmetry within the outer regions. It does not present clear signs of active merging activity or significant tidal disturbances. The color gradient suggests a stellar population that is dominated by older stars. No obvious dust lanes or prominent star-forming regions are visible within the image. Overall, the galaxy appears to be a relatively evolved system with a substantial stellar mass and low ongoing star formation.
