The galaxy exhibits a predominantly smooth morphology, suggesting it may be an elliptical galaxy. The central region displays a bright, concentrated luminosity profile. The outer regions of the galaxy appear fainter and somewhat more irregular in shape. There is evidence of disturbances in the morphology, with some features suggesting a possible interaction or merger event. The overall color suggests the presence of an older stellar population, though bluer regions may indicate ongoing star formation. The galaxy is roughly elliptical in shape. There appear to be signs of a possible ongoing merger.
