This galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that is somewhat luminous, suggesting a high stellar density within this region. The galaxy displays a gradual decrease in surface brightness from the center outwards. No distinct spiral arm structures or significant dust lanes are apparent, hinting at a lack of ongoing major star formation. The overall color is yellow-red, potentially indicating an older stellar population. There are no obvious signs of recent or ongoing merger activity or major tidal disturbances.
