This galaxy presents a complex morphology. It appears to be a system possibly undergoing a minor merger, or displaying tidal disturbances. The main body of the galaxy exhibits a somewhat smooth structure, but there is evidence of a fainter, elongated component extending from one side. This extension suggests potential tidal interactions or an elongated disk. There are hints of a disrupted spiral arm structure within the disk. The color distribution appears relatively uniform across the main body, with a slight shift towards bluer colors in the outer regions of the disk and in the fainter extension. This may indicate ongoing star formation in these regions. However, given the data on artifact fraction, this could also be related to observational artifacts in the image. 
