SFHs of LEWIS galaxies and stellar kinematics properties. Galaxies are separated according to the kinematic type as described in Paper II: Presence of rotation (left panel) vs. non-rotating objects (right panel). Thick solid lines correspond to the average SFH for each panel, and shaded lines correspond to the standard deviation of the distribution. Similarly to Fig. 3, the grey lines correspond to t₅₀ and t₉₀, respectively.