The galaxy presents as a centrally concentrated elliptical, with a smooth morphology. The core exhibits a bright, yellowish-gold hue, suggesting a population of older stars. Radially outward from the core, the light gradually diminishes and transitions to a more diffuse, reddish color. There appears to be minimal indication of spiral arm structure, and no significant dust lanes are discernible. The overall shape appears nearly circular. There are no obvious signs of recent or ongoing major mergers, though some slight asymmetry in the outer regions cannot be ruled out as evidence of minor tidal interactions. Star formation appears to be greatly reduced, possibly entirely absent.
