This galaxy exhibits a morphology that appears to be undergoing a significant interaction, possibly a merger. The primary body of the galaxy is characterized by a diffuse, extended halo of light. Within this halo, two distinct, bright nuclei are visible, suggesting either two galaxies in the process of merging or a single galaxy with an active galactic nucleus and a region of intense star formation. A prominent tidal feature extends away from the main body.

The light from this galaxy indicates ongoing star formation within the system. The system is relatively massive with a significant rate of star formation. The galaxy shows a mixture of colors, with some regions appearing more blue/green, indicative of younger, hotter stars, and other areas exhibiting a reddish hue, possibly due to older stellar populations or dust obscuration. Overall, this appears to be a dynamically active system with ongoing processes shaping its structure.
