The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge characterized by a yellowish hue, suggesting an older stellar population. The galaxy appears generally symmetric, with a slight elongation along what could be considered its major axis. The outer regions of the galaxy fade gradually into the background, with a subtle halo of diffuse light surrounding the brighter core. There's no readily apparent evidence of spiral arm structure, dust lanes, or strong tidal interactions. A slight asymmetry in the extended halo might indicate minor disturbances, but overall, the galaxy appears relatively undisturbed and relaxed. The overall color profile indicates a population dominated by older stars.
