The galaxy presents as a relatively smooth, elliptical-like structure. A bright central bulge dominates, characterized by a concentrated emission of light, which seems to decline gradually toward the outer regions of the galaxy. There is not a strong presence of spiral arm structures or dust lanes, implying it could be a more evolved system. The overall color appears to be slightly reddish, indicating an older stellar population throughout the galaxy, especially the bulge. The light distribution seems to be symmetrical. The galaxy exhibits a high degree of central concentration with a smooth transition between the bulge and the outer regions. It appears to be relatively isolated, not showing signs of recent interactions. The overall morphology suggests a classification as an elliptical galaxy.
