The galaxy appears to be undergoing a significant merging event. Several distinct, luminous cores are visible within a common, diffuse halo. These cores exhibit variations in color, with some appearing redder, suggesting older stellar populations or higher dust content, and others showing a bluer, younger population. The overall structure is highly disturbed, with a lack of clear spiral arm structure or a smooth elliptical profile. There are tidal features such as faint, extended plumes or streamers of light that are indicative of ongoing gravitational interactions. Based on the colors, the galaxy is possibly experiencing moderate amounts of star formation, concentrated in the separate cores. 