The galaxy presents as a relatively small, elliptical-like structure. It exhibits a smooth, centrally concentrated luminosity profile with no apparent spiral arm features or dust lanes discernible at this resolution. The overall color appears redder than the background, potentially indicating an older stellar population and suppressed star formation. The galaxy seems somewhat elongated, with a noticeable cigar shape. There are no obvious signs of a major merger event or significant tidal disturbances in its immediate vicinity, suggesting it is likely a relatively undisturbed system. 
