The galaxy presents as a centrally concentrated, largely smooth, and rounded structure. Its overall color appears to be a yellowish-white, indicative of an older stellar population with fewer young, hot stars. There is a subtle color gradient, with the central region appearing more yellowish-white and the outer regions exhibiting a slightly bluer hue. There is no significant dust lane or spiral arm structure visible. The galaxy's smooth morphology suggests it is likely an elliptical or lenticular type. There is no evidence of any major tidal disturbances or ongoing mergers. The general lack of discernible features is consistent with a relatively quiescent star formation history.
