Photometric decomposition of MUSE collapsed i-band image of galaxy HE 1108−28138. From left to right: data image, model, residual=data-model, and surface brightness profile from isophotal fitting. The colour map in the residual image is stretched to show faint details. The surface brightness profiles in the right-most panel show a separation into all components that were included in the fit. The thick coral line shows the sum of all model components and the black line the observed data. A set of figures that shows the decomposition of the complete sample can be found in the Appendix C.