This galaxy exhibits a morphology indicative of a late-stage merger or strong interaction between two spiral galaxies. The primary body shows evidence of significant tidal disruption, with extended, diffuse stellar structures reaching beyond the main disk. Traces of spiral arm structures can be observed, though heavily distorted. There appears to be some strong star formation activity, particularly in the regions where the two galaxies cores are closest. It has a prominent bulge, which appears to be surrounded by a moderate disk. The system's shape suggests it is not edge-on, but at an inclined angle.&#x20;
