This galaxy presents as a relatively smooth, elliptical-like structure. The light distribution appears centrally concentrated, with a gradual decrease in intensity outward from the core. The core region exhibits a yellowish hue, potentially indicative of an older stellar population. There is little evidence of spiral arms or significant dust lanes. It appears to be an isolated galaxy, as there are no obvious signs of tidal interactions or ongoing mergers. Overall, the morphology suggests a quiescent galaxy dominated by older stars.
