The galaxy exhibits a disk morphology, although with a notable degree of disturbance. The structure appears slightly asymmetric. There is evidence of spiral arms, albeit somewhat disrupted. A hint of a bar structure is present within the central region of the disk. The bulge appears small and not particularly prominent relative to the disk. Evidence suggests ongoing or recent interactions with another galaxy, potentially a minor or major merging event with another galaxy. The central region of the galaxy may display a relatively low rate of star formation. The overall color suggests a population of older stars with only moderate recent or ongoing star formation.
