The galaxy presents a centrally concentrated, elliptical morphology, with a dominant smooth component. A distinct color gradient is observed, transitioning from a yellowish-white core to a bluer periphery. Faint, diffuse extensions are present, suggesting the presence of a stellar halo. There is some low level evidence of a feature possibly indicative of a disk structure. The light distribution is generally symmetric. There is no visually obvious evidence of strong tidal interactions or recent major mergers, though there may be some minor disturbances present.
