The galaxy presents as a disrupted spiral system, exhibiting significant morphological disturbances indicative of an ongoing or recent merger event. The primary structure consists of two prominent luminous cores, likely representing the nuclei of the merging galaxies. These cores display a yellow-orange hue, suggesting an older stellar population. The overall morphology is asymmetrical, with tidal tails extending outwards, a common feature in interacting galaxies. Patchy regions of blue light are observed, indicating areas of active star formation. The system lacks a clear central bulge, displaying instead a more diffuse distribution of light. The spiral arms appear distorted and ill-defined, further supporting the hypothesis of a merger disrupting the galaxy's original structure. The color gradients across the galaxy suggest variations in stellar populations and dust content, with bluer regions corresponding to younger stars and redder regions associated with older stars and dust.
