The galaxy presents as a relatively smooth, elliptical object with a concentrated central bulge. The overall shape appears nearly circular. There is a slight color gradient visible, trending towards redder hues in the central regions, potentially indicative of an older stellar population. A faint extended halo is barely perceptible around the central structure. There are no obvious signs of prominent spiral arms or significant dust lanes, or any major mergers, suggesting it is a relatively undisturbed system. Any disk if present, is not visible. The lack of clear blue regions suggests a low star formation rate. Overall, the galaxy appears to be a fairly evolved system dominated by older stars.
