The galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated luminosity profile with a diffuse, extended halo. The core region displays a yellowish-white hue, possibly indicative of an older stellar population dominating the central regions. Moving outward from the core, the color transitions to a bluer tint, suggesting the presence of younger stars in the outer regions or potentially some ongoing, though limited, star formation. The overall shape is somewhat rounded, with a slight elongation. There are no readily apparent signs of strong tidal interactions or major disturbances in the surrounding structure. A minor asymmetry or slight warping may exist, but further investigation is required to confirm. The galaxy appears to be relatively isolated, with no obvious companion galaxies in close proximity.
