The galaxy presents as a fairly smooth, elliptical-like structure. Its overall color is yellowish, indicating an older stellar population. The central region exhibits a brighter concentration of light. There is a slight elongation, but the overall form appears predominantly rounded. No distinct spiral arms or significant dust lanes are discernible. The outer regions fade gradually into the background sky, without sharp edges or tidal features. There is no obvious sign of any ongoing major mergers or strong gravitational disturbances, though there may be slight irregularities. The color suggests minimal current star formation.
