The galaxy presents as a relatively smooth, elliptical-like structure with an apparent elongation. The central region exhibits a brighter, more concentrated light profile, suggestive of a distinct galactic nucleus. Surrounding this core, a more diffuse halo is visible, fading gradually into the background. The color distribution appears subtly varied. A central reddish hue transitions outward to a greenish-blue tint in the outer regions, implying the possible presence of varying stellar populations or dust distribution. The shape is not perfectly symmetrical. There is a slight disturbance in the otherwise smooth structure, hinting at a possible past interaction or minor merger event. Overall, the morphology suggests an evolved system, potentially with ongoing, low-level star formation.
