Alternative fits to the blue and red bump in M4327. The best-fit models to the combined spectral regions hosting the blue and red bumps are built from a combination of LMC empirical templates from Crowther et al. (2023). While all models contain WN stars, each row differs for the set of complementary templates adopted, namely Of/WN, WNE/C and WNE/L, and WO for the upper, middle, and bottom panels, respectively.