The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing largely round. There is a bright, somewhat diffuse central bulge region that appears yellowish-white in color. The outer regions of the galaxy fade gradually into the background sky, displaying a bluer hue compared to the central bulge. No distinct spiral arms or bar structures are discernible, suggesting a lack of significant ongoing star formation in a disk-like component. There is no visible evidence of any major mergers or tidal disturbances affecting the galaxy's overall structure. Overall, the galaxy presents a regular, relaxed appearance indicative of a mature stellar population.
