The object presents as a galaxy undergoing a significant interaction or merger. Its morphology is highly disturbed, exhibiting no clear spiral arms or elliptical structure. There appears to be two distinct nuclei, with tidal tails extending from the primary galactic body, suggesting an ongoing or recent merger event. The light distribution is uneven, with clumps of brighter regions indicating areas of enhanced star formation, especially between the two nuclei. The color gradients suggest a mixture of stellar populations, with bluer regions potentially indicating younger, hotter stars, and redder regions potentially indicating older populations. There are faint wisps and extended structures that might be tidal debris, further supporting the merger hypothesis. The overall appearance is amorphous and irregular, lacking any well-defined galactic disk or bulge.
