The galaxy appears to be undergoing a major merger event. There is a bright central region, possibly the combined nuclei of the merging galaxies. The galaxy's overall morphology is highly disturbed and asymmetrical, with significant tidal features and distortions indicative of strong gravitational interactions. The color gradient suggests varying stellar populations across the galaxy. The lower portion of the galaxy exhibits a yellowish-orange hue, which could indicate an older stellar population or increased dust obscuration. Towards the upper portion, a blueish tint is observed, possibly indicating areas of active star formation.
