The galaxy presents an elliptical morphology, appearing largely smooth and spheroidal. The central region exhibits a higher surface brightness, with a concentrated core. The overall color profile appears relatively uniform, with a subtle color gradient toward the center, suggesting a slightly bluer population in the core. The galaxy is relatively isolated and shows no obvious signs of recent major merging activity, although there may be a slight asymmetry to the light distribution. The estimated half-light radius indicates a moderately sized galaxy, neither exceptionally large nor particularly compact.
