The galaxy presents a complex morphology suggestive of an ongoing or recent interaction or merger event. A disk component is visible with indications of spiral arm structure. However, the arms appear somewhat disrupted and asymmetric. There is an elongated central bulge, possibly in the beginning stages of tidal disruption. Some regions exhibit bluer colors, indicative of recent star formation, while others appear redder, suggesting older stellar populations. There are noticeable disturbances within the galaxy's structure, including asymmetric light distribution and potential tidal features, that indicate gravitational interactions with another galaxy. Overall, the galaxy presents a disturbed morphology which implies that it is an interacting spiral galaxy undergoing or having recently experienced a merger.
