The galaxy appears as a centrally concentrated object with a roughly elliptical morphology. Its core region presents a yellowish hue, suggesting an older stellar population. Fainter, diffuse extensions are observed, displaying a bluer tint, which potentially indicates the presence of ongoing star formation. There is a slight suggestion of a disc-like structure. Faint asymmetries or disturbances are apparent in the outer regions, possibly indicative of past or ongoing minor interactions.
