The galaxy exhibits a disturbed morphology, indicative of an ongoing or recent interaction. A prominent central bulge is visible, appearing relatively bright and concentrated. Faint spiral arm structures extend outwards, but are distorted and disrupted, particularly on one side, suggesting a potential merger event. Patches of active star formation appear within the disturbed arms and throughout the disk. The overall color suggests a mix of stellar populations, with the bulge having a more yellow/red color characteristic of older stars, while the arms show a bluer hue due to the presence of younger, hotter stars. The galaxy is not a pure disk, and exhibits more irregular shapes. There is a prominent irregular blob on one side, which is brighter and separated from the disk.