Left panel: RGB image of the KLAMA system (Red = F444W, Green = F277W, Blue = F200W). For reference, the yellow square marks a (3″ × 3″) area. We indicate the three components of the galaxy group with capital letters (A, B, and C). KLAMA is the reddest source (A). Right panel: F356W highly contrasted image of the same region shown in the left panel. The three components are indicated. Interestingly, a diffuse emission clearly rises as a bridge (marked with the red arrow) connecting the main system (A+B) to the tail (C). The green circles represent the apertures (equal to the FWHM of the F444W PSF) and the positions used to extract the photometry for the Bagpipes fit.