The galaxy presents as a relatively smooth, elliptical structure with a noticeable bulge. It exhibits a yellowish-orange hue in the central region, suggesting a population of older stars and a lack of significant recent star formation in the core. Moving outward from the center, the color gradually shifts towards a slightly bluer tone, which might indicate the presence of younger stellar populations or perhaps some ongoing, albeit subdued, star formation in the outer regions of the galaxy. The overall shape is elongated, but not exceptionally so, leaning toward an elliptical morphology. There are no readily apparent signs of strong tidal disturbances or ongoing major mergers, although there appears to be a faint asymmetric feature in the halo. The galaxy appears relatively isolated, without any obvious companion galaxies or significant interactions with other nearby structures. 
