Stellar population maps of FCC 167. Top left panel: age map, as measured from pPXF, where a relatively older central component is clearly visible. The metallicity (top right) and the [Mg/Fe] (bottom left) maps show the clear signature of a chemically evolved disk, confined within a vertical height of ∼10 arcsec, which coincides with the kinematically cold component observed in this galaxy (Sarzi et al. 2018b). The IMF map on the bottom right exhibits a different 2D structure, however, that does not follow the metallicity variations, but closely follows the hot+warm orbits of this galaxy (Sarzi et al. 2018b).