2D maps of different components of each galaxy. The model includes an old stellar bulge and disc component, a young non-ionising and ionising stellar disc, as well as a dust disc. The bulge image has been generated with SKIRT using a Sérsic profile geometry. The resolution of each map is based on the respective observations. The extent of the different components is due to the exclusion of unphysical pixels based on the different signal-to-noise ratio (S/N) in each band. The colour coding is in log scale and reflects a normalised flux density.