This galaxy exhibits a disturbed morphology, suggestive of an ongoing or recent interaction or merger. The central region shows a brighter, more concentrated luminosity profile, possibly indicating a galactic bulge or nucleus. However, the overall shape is irregular and asymmetric. The structure seems dominated by a disk, albeit one that is highly disturbed. There are clear signs of tidal features, with elongated extensions of light extending from the main body. No defined spiral arms are visible; instead, the disk appears fragmented and chaotic, with a clumpy distribution of light. The galaxy exhibits a blueish color, potentially indicating a population of young, hot stars, which may be associated with the triggering of star formation due to the merger event. The edges of the galaxy are diffuse. There may be some dust obscuration but it is hard to tell.
