The galaxy presents as a fairly smooth, elliptical morphology. It appears to be relatively round in shape, showing little to no signs of a disk structure. The central bulge is prominent and appears to be quite luminous. The color profile seems relatively uniform across the galaxy, with a yellowish hue. This suggests a stellar population dominated by older, redder stars, and a correspondingly low rate of active star formation. There is no visual evidence of spiral arms, dust lanes, or ongoing mergers or major disturbances. The outer regions of the galaxy fade gradually into the background sky, indicating a smooth density profile.
