The galaxy presents as a relatively smooth, centrally concentrated object. The central region exhibits a yellowish-white hue, suggestive of an older stellar population. Moving outward from the core, the color transitions to a bluer and more diffuse appearance. The morphology is largely elliptical, with a moderate degree of elongation. There is a subtle hint of a disk-like structure, although poorly defined. Minor disturbances may be occurring based on the irregular outer edges, but no major mergers or tidal features are immediately apparent in the image. Overall, the galaxy appears to be an intermediate-mass system with characteristics of a transitioning elliptical galaxy.
