The galaxy exhibits a disturbed morphology, appearing as a system undergoing or having recently undergone a significant interaction. The main body of the galaxy appears elongated, with a tidal tail extending from one end. The tail exhibits a diffuse, bluish color suggestive of ongoing star formation within the disrupted material. The central region shows a concentration of older stars, appearing more yellow in color. A secondary concentration of light can be seen near the opposite end of the main galaxy body. This secondary concentration could be another galaxy involved in the interaction, or a clump of material being disrupted by tidal forces. The overall appearance is suggestive of a system that is not yet completely merged, but where significant gravitational interactions are actively reshaping the galactic structure and triggering star formation. The system displays notable features indicating recent or ongoing tidal interaction and potentially an ongoing merger event.
