The galaxy presents as a fairly smooth, elliptical-like structure with a concentrated central bulge. There is no discernible spiral arm structure. It appears largely featureless, lacking significant dust lanes or prominent star-forming regions. The light distribution suggests a centrally concentrated mass profile. The overall color appears somewhat red, possibly indicative of an older stellar population with lower ongoing star formation. There are no obvious signs of tidal disturbances or ongoing mergers. The galaxy's morphology seems relatively undisturbed.
