The galaxy presents as a system undergoing a significant interaction, likely a merger event. It exhibits an irregular morphology with a disturbed disk. There appear to be multiple distinct luminous clumps within the galaxy, suggesting either multiple nuclei or regions of intense star formation triggered by the interaction. The overall color is dominated by a yellowish hue in the central regions, which potentially indicates an older stellar population or dust obscuration. Bluer regions are also visible, perhaps indicative of younger stars. Tidal features such as faint tails or bridges of material are not immediately obvious in the image, but this may be due to the imaging depth. The galaxy appears slightly elongated but does not exhibit a clearly defined spiral or elliptical structure. There are signs of recent or ongoing star formation, although the rate is unlikely to be exceptionally high.
