The galaxy appears as an elliptical structure with a smooth, diffuse light distribution. The color is predominantly yellowish-orange, suggesting an older stellar population with fewer hot, young stars. The galaxy appears to be relatively regular in shape, without obvious signs of strong tidal interactions or recent mergers. There is a slight elongation visible, indicating that it is not perfectly spherical and may be more of a flattened spheroid. The absence of distinct spiral arms or prominent dust lanes reinforces the classification as an elliptical galaxy. Some bluer regions can be seen towards the edges of the galaxy, potentially indicating very low levels of recent star formation. Overall, the galaxy seems to be a relatively quiescent system.
