The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy at a moderate redshift. It exhibits a bright central bulge that fades gradually into a diffuse halo. There is little evidence of prominent spiral arms or distinct dust lanes, suggesting a relatively old stellar population. The galaxy is somewhat rounded in appearance, although not perfectly spherical. There is a very slight hint of a disk like structure. The color indices suggest the galaxy is composed of older, redder stars. No obvious major mergers or tidal disturbances are apparent in the image, although there may be signs of minor interaction on the outskirts of the galaxy. The star formation rate appears very low. The object is relatively small in angular size on the sky.
