The galaxy presents as a single, concentrated luminous region. Its light profile appears relatively smooth and elliptical, with a high degree of central concentration, transitioning to a gradual decrease in luminosity outward from the core. There is a noticeable color gradient, where the center of the galaxy exhibits a yellowish-white hue, likely indicating a population of older stars. The outer regions appear slightly redder. There are no apparent spiral arm structures or prominent dust lanes visible in this image. The overall morphology suggests a likely early-type galaxy. The galaxy seems largely undisturbed, with no clear signs of recent major merger activity.
