This galaxy appears to be a relatively bright, centrally concentrated system. It exhibits a smooth, elliptical morphology with a noticeable bulge. There is a discernible color gradient, with the central region appearing more yellow/orange, potentially indicating an older stellar population. The outer regions are bluer, suggesting the presence of younger, hotter stars and possibly ongoing star formation. However, no distinct spiral arm structure is visible. There are subtle asymmetries present, indicating a minor gravitational disturbance or interaction with a smaller object. The overall structure indicates that it is not experiencing a major merger. The galaxy is slightly elongated in shape, with the majority of its light being centrally concentrated.
