This galaxy appears to be undergoing a merger, or experiencing significant tidal disruption. Its shape is elongated and asymmetrical, presenting a 'cigar' shaped morphology. There is a clear distortion in its structure, with an apparent secondary nucleus or region of high stellar density offset from the main body. The color gradient shifts from a bluer hue in the disturbed area to a more yellow-orange core, suggesting a difference in stellar populations. Star formation is likely occurring in the bluer regions. The system does not display a well-defined spiral structure.
