The galaxy presents as a somewhat diffuse object, exhibiting a roughly elliptical morphology. Its core region appears comparatively bright and condensed. There is a smooth transition from the central bulge to the outer regions of the galaxy, which are less well-defined and appear fainter. Some slight disturbances may be present, but the galaxy as a whole appears relatively undisturbed. The overall color appears to be consistent with an older stellar population, trending towards the redder end of the spectrum. There is an apparent lack of significant, distinct spiral arms.
