The galaxy appears as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that fades into an extended, diffuse halo. There is a slight elongation, indicating it may not be perfectly spherical. There is a faint, seemingly disturbed arm or tidal tail emanating from one side. Color gradients show a redder core region and a bluer outer disk. Overall, the galaxy appears to be relatively isolated with only minor disturbances in its morphology. 
