The galaxy appears to be a relatively smooth, centrally concentrated object. It has a generally elliptical morphology, with no discernible spiral arms or bar structure. The central region exhibits a yellowish hue, potentially indicating an older stellar population. Moving outward from the center, the galaxy appears to transition to a bluer color, which may be indicative of a younger stellar population or ongoing star formation in the outer regions. The overall color gradient suggests a possible inside-out formation scenario. There are no obvious signs of strong tidal interactions or major mergers. Faint, diffuse extensions are present surrounding the central region, suggesting a halo of older stars. The galaxy displays no pronounced dust lanes. Overall, the galaxy appears to be a relatively quiescent system, likely an elliptical galaxy undergoing passive evolution.
