This galaxy presents as an elliptical morphology, appearing generally smooth and well-rounded. It exhibits a concentrated central bulge with a gradual decrease in luminosity outward towards the edges of the galaxy. The core region displays a yellow-white hue, suggestive of an older stellar population. The outer regions have a more diffuse and reddish tint, potentially indicating the presence of dust or a less dominant population of younger, bluer stars. There is no clear evidence of spiral arms, significant dust lanes, or ongoing major merging activity in the visible structure. The overall form indicates a galaxy which has likely undergone significant dynamical relaxation, suggesting it is in a relatively late stage of its evolution.
