The galaxy presents as a centrally concentrated elliptical system. The core exhibits high luminosity, with a yellow-white hue, suggesting a population of older stars. The luminosity decreases smoothly and gradually outwards from the center. The overall shape is somewhat irregular, appearing closer to a rounded, yet distorted, structure. There is no evidence of spiral arm structure, or a prominent disk. A slight asymmetry is observable in the outer regions, which could be indicative of a minor gravitational interaction or past merger event, however there is no large scale tidal disturbance. The galaxy appears fairly smooth and featureless in structure.
