The galaxy presents as a relatively smooth, elliptical morphology. Its light profile appears centrally concentrated, with a gradual decrease in intensity towards the outer edges. The core exhibits a yellowish-white hue, suggesting an older stellar population. There's a subtle color gradient extending outwards, transitioning to a slightly greener tint in the outer regions, which may indicate pockets of ongoing star formation or a younger stellar population. The overall shape is elongated, hinting at a triaxial structure. No distinct spiral arms or prominent dust lanes are visible. The structure appears largely undisturbed, with no signs of major mergers or tidal disruptions.
