The galaxy presents as a largely featureless, elliptical-like structure. The central region exhibits a bright, concentrated core, indicating a high density of stars. The light profile appears smooth, with a gradual decrease in brightness moving outward from the core. There is a slight elongation, not perfectly spherical. No distinct spiral arms or dust lanes are discernible. The overall color of the galaxy seems to be biased towards redder wavelengths, suggesting a population of older stars and minimal ongoing star formation.
