The galaxy exhibits an elliptical morphology, appearing largely smooth and centrally concentrated. The core region displays a yellowish-white hue, suggesting a population of older stars. A subtle color gradient is observed, with the outer regions exhibiting a slightly bluer tint, possibly indicating the presence of younger stellar populations or ongoing star formation, albeit at a modest rate. No distinct spiral arm structures or prominent dust lanes are discernible within the galaxy's disk. The overall appearance suggests a relatively evolved system, potentially undergoing passive evolution. There is no indication of major mergers or significant tidal disturbances. A slight elongation is observed, with the galaxy shape being somewhere between round and oval.