The galaxy presents a complex morphology, appearing as a system undergoing a significant interaction or merger. The central region exhibits a bright, relatively smooth component, possibly indicating an older stellar population or a bulge. This region displays a slightly bluish tinge, suggesting some ongoing star formation. 

Surrounding this central area are multiple distinct clumps of brighter emission. These clumps appear more yellow in color, perhaps indicating a difference in stellar populations, reddening due to dust obscuration, or older bursts of star formation. The overall shape of the galaxy lacks a clear, defined structure, hinting at gravitational disturbances due to the ongoing interaction. The system does not show defined spiral arms but appears more amorphous. Faint tidal features may be present, although the image resolution makes definite confirmation difficult.
