The galaxy exhibits an irregular morphology. It appears to be undergoing a major merger event with at least three distinct luminous clumps visible, suggesting multiple galactic nuclei or dense star-forming regions. The overall color is yellowish, hinting at an older stellar population. The shape is not clearly elliptical or spiral, rather it looks like a disturbance or interaction is taking place within the galaxy. The mass estimate places it as quite massive. The low star formation rate implies that the merging process may be in a later stage. The light emitted indicates a high luminosity overall.
