The galaxy presents an elongated morphology, suggesting a possible disk-like structure viewed at an oblique angle or a possible merger. The galaxy's light appears to be mostly smooth, with subtle variations in color and intensity across its structure. There's a suggestion of a brighter, somewhat detached region at one end, which could indicate an ongoing or recent interaction with another galaxy. Overall, the galaxy's appearance suggests it could be undergoing some form of interaction or disturbance, affecting its overall shape and luminosity distribution. The color suggests ongoing star formation, with some regions appearing bluer than others.
