  The eHWC J1825-134 source is located in the southern sky and has been
recently detected by the HAWC observatory. It presents an hard spectral index
and its gamma-ray flux extends up to energies close to 100 TeV without
significant suppression. Amongst the HAWC sources, it is the most luminous in
the multi-TeV domain and therefore is one of the first that should be searched
for with a neutrino telescope in the northern hemisphere. Using an updated
effective area for the forthcoming KM3NeT detector, we study the possibility to
detect this source within ten years of its running time. We conclude that about
a 4 to 5 sigma detection has to be expected after ten years of observations,
depending on the details of the considered scenario.
