The galaxy presents as a relatively smooth, centrally concentrated light distribution. It appears elliptical in shape, with a high degree of circularity. The central region is bright and yellowish, suggesting an older stellar population. There is a faint, diffuse halo extending outward from the core, exhibiting a subtle color gradient from yellow to red. No distinct spiral arms or dust lanes are discernible within the image. There are no obvious signs of a major ongoing merger or strong tidal disturbances, although the possibility of a minor disturbance cannot be ruled out due to image resolution. Overall, the galaxy appears to be a massive system with low star formation activity.
