This galaxy appears to be a relatively smooth, elliptical-type system. Its overall shape is somewhere between round and elongated. The light distribution suggests a central bulge that is bright and concentrated, surrounded by a more diffuse halo. Faint blue regions may indicate pockets of star formation, although the dominant color is yellowish, implying an older stellar population. There is no obvious spiral structure or strong evidence of a recent major merger event. A possible faint tidal tail or other minor disturbance could be present. The estimated mass range is around 10^10 solar masses and a relatively low star-formation rate may be present.
