The galaxy presents as a system undergoing a significant interaction or merging event. There appear to be at least three distinct luminous components within the galaxy. Two components are relatively compact and bright, displaying a yellowish hue, suggesting older stellar populations. The third component is more diffuse and elongated, with a fainter, more reddish color, indicating a region with ongoing star formation or a significant dust content. The overall morphology is irregular, with no clear spiral arms or elliptical shape. The galaxy shows some tidal tails and distortions, indicative of gravitational forces from an interaction or merger.
