The galaxy appears as a moderately bright, centrally concentrated elliptical, approximately 9 kpc in radius. Its overall shape is somewhat elongated, but generally smooth. Color gradients are present, with a redder core indicative of an older stellar population and a bluer outer halo. The smoothness of the light distribution suggests a lack of significant ongoing mergers or tidal disturbances, as supported by its apparent shape. The overall color and morphology suggest a relatively evolved system with moderate star formation. 
