The galaxy appears to be a disk galaxy, viewed at a moderate inclination. It exhibits a prominent central bulge, appearing smooth and yellowish-white. The disk component shows some evidence of spiral structure, but it is not highly pronounced; the arms are rather diffuse. The galaxy's color profile suggests an older stellar population dominating, with a less prominent blue component which indicates a low level of ongoing star formation. The overall shape is elliptical, but approaching round. There is no obvious evidence of a major merger or tidal disturbances.
