The galaxy presents a somewhat irregular morphology, suggesting potential interactions or recent mergers. The central region shows a concentration of light, but not a pronounced, distinct bulge. There is evidence of a disk component. The disk exhibits faint spiral arm structures, though they appear somewhat disorganized and patchy. Patches of bluer light are observed throughout the disk, possibly indicating regions of active star formation. There is no strong evidence of a prominent bar structure in this image. Overall, the galaxy appears to be experiencing some form of gravitational disturbance, as evidenced by its irregular shape and fragmented spiral arm patterns. It could be undergoing a minor or major merger.
