The galaxy presents as a relatively smooth, elliptical-shaped object with a concentrated central bulge. There is a lack of prominent spiral arm structure or significant dust lanes. The light is predominantly yellowish-white, indicating an older stellar population. The galaxy appears to be relatively isolated, showing no clear signs of tidal interactions or ongoing mergers, though a slight asymmetry could suggest minor past disturbances. Its overall morphology suggests it is likely a mature system, possibly an elliptical galaxy, with a low rate of star formation.
