Left: Stellar mass–halo mass relation for the galaxies in our samples. For comparison, we show the empirical fit by Moster et al. (2018) with a dashed black line along with individual fits of such a relation to each of our samples (solid blue, dot-dashed green, and dotted red for mostly-discs, intermediate, and spheroidals, respectively). There is a clear morphological trend in the relation, with disc-dominated objects populating haloes with two to ten times lower mass than spheroid-dominated objects at the same M_⋆. Similarly, at fixed M₂₀₀, disc-dominated galaxies form more stars than spheroids. Right: Distribution of the median stellar age of the galaxies in each subsample. We found a systematic trend with morphology where the disc-dominated samples are on average younger than the spheroid-dominated galaxies.