Stellar population in the MUSE FoV. Top panel: extinction-corrected Hα map with the location of YSCs of age ≤10 Myr (green triangles). Bottom panel: enlargement of one of the H II region complexes. Green triangles indicate the position of YSCs observed with HST (Adamo et al. 2015), blue crosses and red stars indicate respectively WR stars and PNe identified in the MUSE dataset and orange squares are SNR from Long et al. (2022).