The galaxy presents a largely smooth, elliptical morphology. The central bulge appears bright and concentrated, exhibiting a yellowish-white hue, suggesting a population of older stars. Moving outward from the core, the light gradually diminishes, transitioning to a bluer shade. This outer region lacks any clearly defined spiral arm structures or prominent dust lanes. There is a subtle hint of minor disturbances, but no clear indication of a major ongoing merger event. Overall, the galaxy appears as a relatively undisturbed, mature system.
