The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. There is a distinct color gradient, with the core exhibiting a yellowish-white hue, indicating an older stellar population. The outer regions of the galaxy are less defined and show a slightly bluer tint, hinting at the presence of some younger stars. The overall shape is nearly circular, with only a very slight elongation visible. There is no apparent evidence of spiral arms, dust lanes, or active galactic nuclei activity from visual inspection. The galaxy appears to be relatively isolated, with no immediate signs of ongoing mergers or major tidal disturbances.
