The galaxy presents as a primarily smooth, somewhat elliptical structure. A centrally concentrated bulge dominates the luminosity profile, exhibiting a yellowish hue. The outer regions of the galaxy appear more diffuse, with a transition to bluer colors. There are faint, subtle features that may be indicative of a disk component, but they lack defined spiral arms. Overall, the galaxy appears relatively undisturbed, with no obvious signs of a major merger. Some minor disturbances or asymmetries are visible in the outskirts of the galaxy.
