The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a high concentration of light, appearing as a bright, relatively uniform core. There is a noticeable decrease in luminosity as one moves radially outward from the center. The galaxy appears nearly round, with minimal elongation discernible. No distinct spiral arm structures or prominent dust lanes are visible. Faint, diffuse features may exist in the outer regions, though these are not well-defined, possibly indicating minor disturbances. Overall, the galaxy appears to be a relatively undisturbed system.
