Measured RAR of the KiDS-bright isolated lenses (points with 1σ error bars) divided into canonically early- and late-type galaxies. In the left panel, the lenses are split by Sérsic index (n ≷ 2) into bulge-dominated (red points) and disc-dominated (blue points) galaxies. In the right panel they are split by u − r colour (m_u − m_r ≷ 2.5) into red and blue galaxies (with correspondingly coloured points). In both panels we find a significant difference between the RAR measurements of early and late galaxy types. The extrapolated MOND and EG predictions (grey solid and red dashed lines) and the SPARC data (red squares with 2D histogram) are shown as a reference.