The galaxy presents as a somewhat rounded, centrally concentrated object. Its light is primarily smooth in appearance, with a slight hint of possible disk-like structure but no obvious spiral arms or significant irregular features discernible in this image. The galaxy appears to be of substantial mass and exhibits a relatively low star formation rate. The observed colors suggest that the galaxy is comprised of an older stellar population. A high degree of central symmetry is present. There is little to no evidence of recent or ongoing mergers or major disturbances affecting the overall structure.
