The galaxy appears to be a smooth, centrally concentrated object. It exhibits a generally elliptical morphology with a high degree of circularity. The luminosity is strongly concentrated toward the core. There is no apparent disk or spiral structure. Faint, diffuse light extends outwards from the central region, fading into the background sky. A very subtle color gradient may be present, with the core appearing slightly bluer than the outer regions. No evidence of strong tidal features or major mergers is observed, though a minor disturbance cannot be ruled out due to low image resolution. The object lacks any obvious dust lanes or prominent star-forming regions. Overall, the galaxy is consistent with an elliptical galaxy type.
