  The low-luminosity Active Galactic Nuclei M87, archetype of Fanaroff-Riley I
radio-galaxies, was observed in a historically quiet state in 2017. While
one-zone leptonic jet models alone cannot explain the core radio-to-gamma-ray
spectrum, we explore a hybrid jet-disc scenario. In this work, we model the
overall spectral energy distribution of M87's core with a dominating one-zone
lepto-hadronic jet component, coupled with the contribution from the accretion
flow. We find close-to-equipartition parameter sets for which the jet component
fits the radio-to-optical data as well as the gamma-ray band, while the
accretion flow mainly contributes to the X-ray band. The effects of gamma-ray
absorption by the Extragalactic Background Light during the propagation towards
Earth are probed and are found to be negligible for this model. The neutrino
flux produced by such scenarios is also calculated, but remains below the
current instruments' sensitivity.
