Similar to Fig. D.1 but showing here multi-component decompositions of core-Sérsic LeMMINGs galaxies (see Table B.4). These galaxies have a central deficit of light relative to the inward extrapolation of their bulge’s outer Sérsic profile. Of the 15 core-Sérsic elliptical galaxies in the full sample, 6 (NGC 0315, NGC 0410, NGC 2832, NGC 3193, NGC 5322, and NGC 6482) have an outer stellar halo component that we modelled with an exponential function.