This galaxy appears to be a spiral galaxy undergoing a significant merger or interaction. The morphology is visibly disturbed, exhibiting disrupted spiral arms. There is an indication of a moderate bulge, surrounded by a disk with patchy regions of star formation. The spiral arms are not well-defined; rather, they appear fragmented and warped, with significant tidal distortions and extended faint structures that indicate ongoing gravitational interaction. The central region appears relatively concentrated and has a yellow/white hue, possibly indicating an older stellar population. The disk displays bluer regions indicative of younger stars. The overall shape deviates significantly from a regular spiral, suggesting a recent or ongoing merger event.
