The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is a noticeable yellow-white hue, suggesting an older stellar population within the galaxy. The galaxy appears to be somewhat compact. There are no obvious signs of spiral arms or prominent dust lanes, reinforcing the likelihood of it being an elliptical galaxy. The overall light distribution seems fairly even, with a gradual decrease in brightness from the center outwards. There is no indication of any major ongoing merger events or significant tidal disturbances.
