This galaxy presents as a fairly smooth, elliptical-like structure. The central bulge exhibits a concentrated, bright yellow-white hue, suggesting a population of older stars. The galaxy's overall shape is quite round, with a gradual decrease in brightness moving outwards from the core, without any distinct features or spiral arm structures. There are no strong indications of a major ongoing merger, although there is a slight asymmetry in its outer regions that indicates there could be a minor interaction occurring. Overall, the galaxy appears to be a fairly evolved system.
