The galaxy presents as a centrally concentrated, smooth object. It exhibits a largely elliptical morphology with a slight elongation, and a diameter on the order of several kiloparsecs. The light distribution is centrally peaked, with a gradual decrease in luminosity outwards. There is no evidence of strong spiral arm features or prominent dust lanes. The galaxy's color is primarily a blend of red and green, tending to purple, with a faint blue outer halo indicating some low-level star formation may be present, though the dominant population appears to be older stars. There is no apparent major disruption due to interactions with nearby objects and the galaxy appears relatively undisturbed. Minor disturbances in the outer edges may hint at a possible minor merger in its past.
