The galaxy presents a mostly smooth morphology, appearing as an elliptical system when viewed from our vantage point. It exhibits a concentrated central bulge, with a gradually decreasing luminosity profile extending outwards. There is a suggestion of a slight disc structure. The color is generally redder, indicating an older stellar population and a low rate of ongoing star formation. No obvious signs of spiral arms or significant dust lanes are visible. There are no signs of recent or ongoing major merger events. There may be a minor disturbance from the image. The galaxy appears generally round.
