The galaxy appears to be an interacting system, potentially in the late stages of a merger. The morphology is complex. One component displays a disk-like structure with some irregular features. It has hints of spiral arms. The colors in this component suggest a mix of stellar populations, with bluer regions possibly indicating ongoing or recent star formation, and redder regions likely populated by older stars. The other component is more amorphous and appears as a smoother, yellowish-orange blob. This may be the remnant of a smaller galaxy that has already largely merged with the disk galaxy, or a dense bulge of an existing system. There are tidal tails, suggesting a moderate amount of gravitational disturbance. Overall, the galaxy exhibits a disturbed morphology, indicative of recent or ongoing interactions.
