The galaxy appears to be undergoing a merger. It presents as a multi-component system, with two distinct, bright nuclei. The primary nucleus exhibits a yellowish-red hue, while the secondary nucleus displays a bluish-white color. There is also some green. These color differences suggest variations in stellar population or dust content between the two.  The overall shape is irregular, indicative of gravitational interactions disrupting the original morphology. A faint, diffuse halo surrounds the central region, hinting at tidal debris or a disturbed stellar population extending beyond the main bodies. There is an indication of possible tidal tails or bridges connecting the two nuclei. This indicates an ongoing interaction process.
