The galaxy presents as a single, relatively smooth concentration of light. Its morphology appears elliptical, with a high degree of central concentration and a gradual decrease in luminosity towards the outer regions. There is no discernible spiral arm structure, bar, or obvious dust lane visible. The color profile suggests a generally older stellar population; the central region exhibits a yellowish hue, while the outer regions are somewhat bluer. The object appears largely undisturbed, with no signs of ongoing major mergers or tidal features. There may be some signs of faint asymmetry in the outskirts, which could hint at minor interactions, but the galaxy predominantly exhibits a relaxed and evolved state.
