The observed galaxy presents a disturbed morphology, possibly indicative of a galaxy interaction or merger event. The galaxy exhibits an irregular shape, with a somewhat bright, bluish central region and a more diffuse, elongated extension to one side, appearing more yellow/red. This extension hints at tidal tails or disrupted spiral arm structures. It appears that the central region shows some degree of smoothness or featurelessness, while the elongated section has a more disturbed appearance. The color gradient observed suggests differential stellar populations, with the central region potentially containing younger, bluer stars, and the elongated section hosting older, redder stellar populations.
