  The radio galaxy M87 is the central dominant galaxy of the Virgo Cluster.
Very High Energy (VHE,$\gtrsim 0.1$ TeV) emission, from M87 has been detected
by Imaging Air Cherenkov Telescopes (IACTs ). Recently, marginal evidence for
VHE long-term emission has also been observed by the High Altitude Water
Cherenkov (HAWC) Observatory, a gamma ray and cosmic-ray detector array located
in Puebla, Mexico. The mechanism that produces VHE emission in M87 remains
unclear. This emission is originated in its prominent jet, which has been
spatially resolved from radio to X-rays. In this paper, we constructed a
spectral energy distribution from radio to gamma rays that is representative of
the non-flaring activity of the source, and in order to explain the observed
emission, we fit it with a lepto-hadronic emission model. We found that this
model is able to explain non-flaring VHE emission of M87 as well as an orphan
flare reported in 2005.
