The galaxy appears to be undergoing a merger or a significant interaction, presenting a disturbed morphology. Two distinct, relatively bright, and slightly elongated central components are visible, potentially representing the original nuclei of the merging galaxies. These components exhibit a reddish-orange hue, possibly indicating a population of older stars or significant dust obscuration. A fainter, greenish glow surrounds these central structures, suggesting areas of more recent star formation activity triggered by the interaction. The overall shape of the galaxy is irregular and lacks well-defined spiral arms or a smooth elliptical profile. There are hints of tidal tails or extended debris structures emanating from the central region, further supporting the interpretation of an ongoing merger event. The galaxy appears relatively compact, with a noticeable concentration of light towards the center.
