The galaxy exhibits a morphology indicative of a system undergoing interaction or merger. A bright, nearly circular central component dominates the image, displaying a smooth appearance with a blue-green hue. Two distinct tidal tails extend outward from this central region, suggesting gravitational disruption. One tail curves prominently towards the right, appearing broader and more diffuse, with a yellow-orange coloration hinting at older stellar populations. The second tail stretches toward the left, appearing fainter and less defined, with a reddish tint. The overall structure hints at a complex interplay of gravitational forces, possibly from a recent or ongoing galactic merger event.
