The galaxy presents as a luminous, yellow-orange elliptical shape, suggesting an older stellar population. The light distribution appears relatively smooth, with a slight elongation. There is a possible core or central concentration of light that is brighter than the surrounding region. A subtle indication of a disk-like structure may be present, but this is not clearly defined. Overall, the galaxy appears to be in a relatively advanced stage of evolution, characterized by a lack of significant star formation activity. The system might be undergoing a minor disturbance, but the overall structure is relatively undisturbed. A merging event is possible, although the primary structure remains relatively intact.
