The galaxy presents as a slightly elongated structure, with an intermediate ellipticity, not quite circular but also not heavily elongated. The galaxy’s light is relatively smooth in distribution across the galaxy's body, with no easily discernable spiral arm structures or dust lanes. This indicates a more spheroidal morphology.

Color gradients exist across the galaxy, with the central region exhibiting a slightly more yellowish or golden hue. The outer regions appear bluer, suggesting that the stellar population is relatively older and more evolved in the center, and contains a population of younger stars in the outer regions. No tidal tails or other signs of major disturbances are observed, however, the existence of the blue outer regions might indicate past minor merger or accretion event. 
