The galaxy exhibits a complex morphology, appearing as a system undergoing, or having recently undergone, a significant interaction or merger. There are multiple distinct nuclei visible, one being more intense than the other, suggesting ongoing tidal forces disrupting its structure. The overall shape of the galaxy is elongated, appearing somewhat cigar-shaped, but with irregularities. The system displays a yellow hue and a red point which may be evidence of an older stellar population with little active star formation currently taking place, which can be confirmed with follow up observations. There is some evidence of a tidal tail extending from the main body of the galaxy, potentially indicative of gravitational disturbances from past or ongoing mergers.
