The galaxy presents as a relatively smooth, elliptical structure with a slightly elongated morphology. Its central region exhibits a concentrated, luminous core, suggesting a high density of stars. A gradual decrease in brightness is observed extending outwards from the center, indicating a lower stellar density in the outer regions. The color gradient displays a shift from yellowish-white in the core to a reddish hue towards the periphery. Faint evidence of a disk structure is present, but this galaxy is not dominated by prominent spiral arms or distinct features. There may be little to no ongoing major star formation. Overall, this galaxy appears to be a relatively undisturbed system with a high degree of symmetry.