This galaxy appears to be undergoing a significant merger event. The primary component exhibits a largely smooth morphology, with a relatively round shape. A secondary component, showing a more elongated form, is situated in close proximity, suggesting gravitational interaction. Color gradients are visible, with the main galaxy body presenting a bluer hue than the secondary component, which has a yellower color indicative of a more aged stellar population. There is a strong indication of tidal distortion affecting the system; overall, the structure is highly perturbed, supporting classification as a merger.
