The galaxy appears as a single, luminous object with a largely featureless morphology. It exhibits a centrally concentrated light profile, with a gradual decrease in surface brightness outwards. Its shape is generally elliptical, tending towards the "in between" class of roundness, showing a slight deviation from a perfectly circular form but not significantly elongated. No distinct spiral arms, bars, or rings are discernible. The overall color appears somewhat redder, implying an older stellar population and/or significant dust content. There are no obvious signs of ongoing mergers or tidal disturbances, and the galaxy appears well-isolated. Its estimated size is relatively compact, with the majority of the light contained within a small radius. 
