The galaxy presents as a somewhat diffuse object with an elliptical morphology. Its color profile appears to be slightly redder in the central region, indicating a potential concentration of older stellar populations or dust obscuration there. The outer regions show a bluer hue, suggestive of ongoing star formation. There is a slight disk-like structure, although it's not well defined. Some mild disturbances or asymmetries are visible. The overall structure shows hints of recent or ongoing interactions.
