The galaxy presents as a merging system, with a complex and disturbed morphology. The main body of the galaxy exhibits an elongated structure, showing some signs of a possible disk-like component. There appears to be at least one companion galaxy involved in the interaction. Evident tidal features, possibly tidal tails or bridges, suggest significant gravitational disruption. There is a brighter, more compact region within one of the merging components, potentially indicating a concentration of star formation or a galactic nucleus. The overall color suggests a mix of stellar populations, with the brighter regions having a bluer hue possibly caused by newly formed stars. Dust lanes are faintly visible, indicating a rich interstellar medium and ongoing star formation. The galaxy shows substantial signs of a significant merger event.
