The galaxy presents as a centrally concentrated, smooth object. Its morphology appears largely elliptical, displaying high degree of circularity with only a slight deviation from a perfect sphere. The light distribution is strongly concentrated towards the center, suggestive of a prominent galactic nucleus or bulge. The galaxy appears to be relatively undisturbed, with no obvious signs of major interactions or mergers. Faint bluer features surround the center, possibly regions of low level star formation.
