The galaxy presents as a centrally concentrated, smooth elliptical galaxy with a noticeable spheroidal morphology. It exhibits a yellowish-orange hue at its core, transitioning to a fainter, greenish-blue in its outer regions. There is no clear evidence of spiral arm structures or significant dust lanes. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal distortions within the visible light spectrum. The light profile gradually fades outwards, suggesting a relatively old stellar population dominating the overall emission. There are no distinct or prominent star-forming regions visible within the galaxy's structure.
