The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. The light profile appears centrally peaked, indicative of a high concentration of stars towards the galactic center. The color indices suggest a relatively red population, particularly in the bulge region, possibly indicating an older stellar population and low current star formation. There is little evidence of spiral arms or significant dust lanes. There appears to be no signs of tidal disturbances or ongoing mergers based on the image. The galaxy's morphology appears relatively undisturbed, and the shape seems quite round.
