The galaxy presents a generally smooth, elliptical morphology. Its light profile appears centrally concentrated. There are some slight color gradients from the center outwards, suggesting variations in stellar populations or dust distribution within the galaxy. The overall color is somewhat red, implying an older stellar population and a relatively low rate of on-going star formation. There does not appear to be any significant tidal features or signs of recent major merger activity. A slight asymmetry or minor disturbance cannot be ruled out based on the image alone, though it seems unlikely.
