The galaxy exhibits a morphology that suggests it is in a merging state. Multiple distinct luminous clumps are visible, appearing to be in the process of coalescing. The overall shape is irregular and lacks a defined structure such as spiral arms or a prominent bulge. The color profile is relatively uniform throughout, with a yellow-orange hue, possibly indicating an older stellar population. There are no obvious dust lanes or regions of intense blue star formation readily apparent in this image. The galaxy is relatively compact, but not perfectly smooth.
