The observed galaxy exhibits a complex morphology indicative of a major merger event. The system consists of two primary components: a lower component that is highly distorted, with an elongated shape and a more concentrated central region suggesting the presence of an underlying bulge. This component displays a reddish hue. The upper component is more diffuse and shows distinct blue coloration, potentially indicative of ongoing star formation. A tidal tail extends upwards from the diffuse component, further suggesting strong gravitational interaction. There are hints of loose spiral structure, but the ongoing merger is disrupting this considerably. The system lacks a clearly defined bar structure. The overall structure of the galaxy is heavily perturbed, lacking smooth features.
