The galaxy presents as an elliptical, likely a spheroidal, system with a smooth, centrally concentrated light profile. There is a bright, unresolved core indicating an active galactic nucleus or a high concentration of stars in that region. The galaxy appears nearly edge-on, or somewhere "in between" round and edge on, as some of the disk may be visible. There is little evidence of spiral arms or prominent dust lanes. The overall color appears to be relatively uniform across the galaxy's extent, suggesting an older stellar population and limited ongoing star formation in the galaxy's disk. There appears to be very little disturbance of the light profile from galactic mergers. The absolute magnitudes are generally on the low end, potentially indicating that this is a low-mass galaxy.