The galaxy appears to be a relatively smooth, elliptical system. The central bulge exhibits a yellowish hue, suggesting a population of older stars. A faint, diffuse halo surrounds the core, showing a slightly bluer tint. This suggests the presence of younger stars. The galaxy appears largely undisturbed. The light distribution suggests a slightly elongated morphology. There is no evidence of strong spiral arm structures or a prominent disk. Overall, the galaxy presents a relatively simple, evolved structure.
