The galaxy appears to be a relatively smooth, elliptical system. Its overall color suggests a population of older stars with a lower rate of ongoing star formation. The central region shows a higher concentration of light, indicative of a significant bulge component. The galaxy displays an intermediate roundness, not perfectly spherical but not highly elongated. No signs of major mergers or significant tidal disturbances are apparent, though there could be some minor perturbations. The galaxy’s morphology suggests it is a fairly evolved system.