The galaxy presents as a relatively smooth, elliptical morphology. The central bulge is a concentrated, bright yellowish-white, suggesting an older stellar population. There's little indication of spiral arms or significant dust lanes, further supporting a classification as an elliptical galaxy. The galaxy's halo appears diffuse and fades gradually into the background sky. There are no obvious signs of a major ongoing merger, tidal tails, or significant disturbance of the galaxy's overall structure. Faint bluer hints in the outer regions suggest some amount of recent star formation. The galaxy appears approximately round in projection.
