The galaxy presents as a primarily smooth, concentrated object with a notable central bulge. Its shape is largely elliptical, appearing only slightly elongated. The galaxy exhibits a yellowish-white hue overall, suggesting a population of older stars. There is some indication of slight asymmetry or minor disturbance in the outer regions, but no clear signs of on-going major merger activity. A faint, diffuse halo may be present, extending beyond the bright core. There appears to be little to no dust obscuration visible. The morphology is consistent with that of an early-type galaxy.
