  GX 301-2 is a high-mass X-ray binary (HMXB) with strong stellar outflows. The
evolution of these binaries can be closely related with the interstellar
environment due to strong wind interactions. We try to constrain the energy
injected in the interstellar medium by GX 301-2 through stellar wind using
HAWK-I and Herschel data. We analysed HAWK-I images in four different filters
(Br$\gamma$, H$_2$, J, and Ks) and tried to retrieve signatures of the impact
of GX 301-2 on its environment. We used Herschel data to outline the
interstellar medium and the Gaia DR3 catalogue to infer the proper motion of GX
301-2. Finally, we estimated the energy injected in the interstellar medium
since the first supernova event of the HMXB. Using both HAWK-I and Herschel
images, we deduce an approximation of the total mass injected from GX~301-2 in
the interstellar medium of $M_{\rm inj} = 3.05 ^{+0.05}_{-0.03} 10^{-2}
M_{\odot}$.
