The galaxy presents as a largely elliptical system, with a smooth, concentrated light profile indicative of an early-type morphology. Its color appears to be generally redder, suggesting a stellar population dominated by older, cooler stars and a lower rate of on-going star formation. The high degree of central concentration in the light distribution is consistent with a substantial bulge component. There is no visually apparent disk structure or spiral arm features. The overall roundness suggests it is closer to an E0 or E1 classification. No major disturbances from interactions with other galaxies are visibly detected; its form appears relatively relaxed and unperturbed.
