The galaxy appears to be a relatively smooth, centrally concentrated system, with a generally elliptical morphology. There is a subtle hint of a disk-like structure or perhaps faint spiral arms, although it's not a strongly defined feature. The light distribution suggests a high degree of rotational symmetry, with isophotes that are generally elliptical in shape. The galaxy exhibits a color gradient, becoming redder towards its center, indicating an older stellar population dominating the core. There are no apparent major mergers or tidal disturbances. Overall, this galaxy is consistent with a high mass system, possibly undergoing quenching of its star formation.
