The galaxy presents a disturbed morphology, indicative of an ongoing or recent merger event. The main body exhibits a somewhat amorphous shape, with a suggestion of a disk-like structure disrupted by gravitational interactions. There is a faint, diffuse component extending outwards from the central region. The color appears to be overall blueish, hinting at the presence of younger stellar populations and ongoing star formation, albeit at a relatively low rate. The galaxy does not appear to have a well-defined spiral or elliptical structure. Patches and a few regions of intense brightness suggests that the merger may be triggering enhanced star formation in localized areas. The galaxy's shape is closer to a round shape than a cigar. There is potential for ongoing tidal interactions or the presence of faint tidal tails not easily resolved in the image.
