The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is ellipsoidal, appearing largely round. The galaxy exhibits a prominent bulge component, which dominates its luminosity profile, with an apparent lack of distinct spiral arm structures. There is a color gradient observed, where the central bulge displays a yellower hue than its outer regions. The overall color suggests a galaxy whose stellar population consists largely of older stars, implying lower levels of on-going star formation activity. There is little evidence of morphological disturbances or interactions, indicating it is likely an isolated system.
