The galaxy presents as a fairly symmetrical, elliptical morphology. It exhibits a smooth light distribution with a concentrated central bulge and a gradual decrease in luminosity toward the outer edges. Coloration appears generally uniform, with a yellow-red hue indicative of an older stellar population and minimal ongoing star formation activity. There is no readily apparent spiral structure, dust lanes, or tidal features suggestive of recent mergers or interactions. The overall structure suggests a relatively relaxed system that has likely undergone significant dynamical evolution.
