The galaxy presents as a system of two primary bodies, likely undergoing a merger or significant interaction. The overall color profile suggests an evolved stellar population, with a yellowish-orange hue dominating both components. The upper body appears relatively smooth and elliptical, exhibiting a concentrated central region that fades into a less defined outer halo. The lower body, while also displaying a smooth texture, seems more elongated or disk-like. A faint, bridge-like structure may connect the two bodies, suggestive of tidal forces at play. The galaxy shows evidence of disturbance in its morphology, likely due to the interaction between the two bodies. Deeper imaging and spectroscopic analysis would be necessary to confirm this merger scenario and characterize the stellar populations within each component.
