The galaxy presents an overall elongated, somewhat irregular morphology. The light profile is brightest in what appears to be a central region, with a diffuse halo extending outward. There is some indication of potential disturbances in the structure of the galaxy. It is exhibiting a blue hue with a brighter, distinct area, possibly representing a region of active star formation. There are possibly two separate nuclei. While there isn't a clear, defined spiral structure, there may be some arm-like features, although any definitive classification is obscured by the galaxy's overall irregular shape. Overall, the galaxy appears to be undergoing some kind of interaction or merger.
