The galaxy exhibits a generally elliptical morphology, appearing as a flattened spheroid. The central region is markedly brighter and more luminous than the outer regions, suggesting a concentration of older stellar populations. The light distribution smoothly decreases in intensity with increasing distance from the center. The galaxy displays a moderate degree of flattening. Its color is a continuum of yellow-to-greenish white. The galaxy appears relatively undisturbed, with no obvious signs of tidal tails or other major interactions. There is a slight asymmetry to the galaxy's shape, possibly indicating a minor interaction or internal structure. The disk, if present, is not easily discernible.
