This galaxy exhibits a morphology indicative of a system undergoing a merger event. It presents as an elongated structure, with two distinct, bright regions. One region displays a more concentrated, nearly spherical shape, suggesting a possible galactic nucleus, while the second appears more diffuse and elongated. There are no obvious spiral arms. The color gradient ranges from bluer hues in the outer regions to redder tones toward the core, hinting at differential star formation or dust distribution. The overall light distribution is relatively smooth. There are tidal distortions in the galaxy's shape. There appears to be ongoing interactions influencing the overall structure of the galaxy, based on the disturbed morphology.
