The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The overall color appears to be slightly yellow or gold tinged, indicative of an older stellar population dominating its composition. There is no evident spiral arm structure or prominent dust lanes within the galaxy's morphology. The galaxy exhibits a high degree of roundness, without noticeable distortions or tidal features. There is no indication of any major ongoing merging activity. The galaxy appears to be quite isolated.
