V-band images of some S0 remnants resulting from minor mergers onto a gS0 galaxy, showing no traces of their past satellite accretion just after ~3 Gyr of total evolution. The bar in these remnants is an evolved version of the one already present in the gS0 progenitor. Warped discs in minor-merger cases are more common than in major mergers. Some of them can be seen in the edge-on views represented here (in particular, models gS0dE0o101 and gS0dS0o102). Notice the bending of the isophotes in their Gaussian-smoothed colour images. For a complete description, see the caption of Fig. 5.