The galaxy appears as a concentrated, elliptical-like structure. The light profile is smooth and centrally concentrated, displaying a gradual decrease in intensity from the core outwards. There is no apparent evidence of spiral arms, a galactic bar, or significant dust lanes. The galaxy exhibits a fairly uniform color profile across its entirety. The morphology suggests an older stellar population and a relatively quiescent star formation history. There are no major visible signs of tidal disturbances, mergers, or other significant gravitational interactions. The overall appearance indicates a mature, relatively undisturbed system.