Two-dimensional light distribution for the dynamical and photometric components of FCC 167. Left panel: two-dimensional distribution of light from each of the dynamical components, as derived from the best-fitting orbit-superposition model shown in Fig. 8: dynamically cold, warm (thick disc), and hot (bulge) componentsare shown in the top, middle and lower panel, respectively. Right panel: two-dimensional distribution of light from each of the photometric components, Sérsic bulge (middle panel) and exponential disc (top panel), as derived from the fit of the light distribution of the MUSE reconstructed image shown in Fig. 4. In the lower panel is shown the resulting image from the superposition of the hot (bulge) and warm (thick disc) dynamical components. In all panels, the colour bar indicates the surface brightness levels adopting an arbitrary zero point.