The galaxy presents as a relatively smooth, elliptical object. The core exhibits high luminosity, suggesting a concentration of older stars and potentially a supermassive black hole. There is a gradual decrease in surface brightness outwards from the core. The overall shape is elliptical rather than a defined spiral, with a high degree of roundness. There are no apparent tidal tails or other major disturbances, indicating the absence of recent major mergers. Faint disk-like features may exist, but the galaxy is not primarily disk-dominated. The colour index suggests a population of older stars with lower levels of recent star formation. There appears to be minimal ongoing star formation within the observed region.
