The galaxy presents as an elliptical morphology, with a smooth, diffuse light profile that decreases steadily from the center outwards. There is little indication of spiral arms or other distinct features. The galaxy exhibits a slightly elongated shape. The central region appears more yellow, potentially indicating an older stellar population or a higher dust concentration. The outer regions show a slight bluish tint indicating the presence of younger stars. Overall, the galaxy seems to be a relatively undisturbed system, appearing well-formed and stable.
