The galaxy presents as a somewhat diffuse elliptical morphology. A prominent, concentrated central bulge exhibits a yellowish hue, indicative of an older stellar population. The outer regions of the galaxy display a bluer tint, suggesting the presence of younger stars and ongoing star formation, although at a comparatively low rate. The overall shape appears relatively smooth, with only subtle irregularities in the outer regions. There is a possible slight distortion in the halo's symmetry. No clear spiral arms or bar structures are discernible. The galaxy displays a moderate size.
