The galaxy appears to be a single, relatively smooth object with a generally elliptical morphology. The light distribution is centrally concentrated, with a gradual decrease in brightness outward. The galaxy exhibits a reddish-orange hue, suggestive of an older stellar population and/or significant dust content. There are no clear spiral arms, bars, or other distinct features typically associated with disk galaxies. The galaxy's overall structure suggests that it is likely an early-type galaxy, possibly an elliptical or lenticular galaxy. There are no obvious signs of any recent major mergers or interactions, though there seems to be a very minor tidal disturbance at the bottom.
