The galaxy exhibits a generally elliptical morphology with a smooth, centralized light distribution. The core region is bright and concentrated, suggesting a high stellar density. The overall color appears yellowish-red, potentially indicating an older stellar population and a relatively low rate of ongoing star formation. There is little evidence of prominent spiral arms or significant dust lanes within the visible spectrum. The outer regions of the galaxy appear to fade gradually into the background, implying a lack of sharp boundaries or distinct structural features beyond the central bulge. The galaxy appears to be relatively undisturbed, showing no obvious signs of recent mergers or tidal interactions.
