The galaxy presents a morphology characterized primarily by a smooth, elliptical-like structure. It exhibits a centrally concentrated light profile, with a gradual decrease in luminosity towards the outer regions. There are no apparent spiral arms or a distinct disk component. The galaxy appears generally round. There is no obvious evidence of a major ongoing merger, or a strong tidal interaction. A slight distortion or minor disturbance cannot be ruled out. It is likely a relatively massive galaxy. The color profile suggests a population of older stars with ongoing star formation.
