  Most of the extragalactic objects detected so far in the very high energy
(VHE) regime are blazars, but the discovered nearby radio galaxies: M87, Cen A
and NGC 1275 of type FRI seem to constitute a new class of VHE emitters. The
radio galaxy PKS 0625-354 was observed and detected ($\sim$6$\sigma$) with the
H.E.S.S. phase I telescopes in 2012, above an energy threshold of 250 GeV. The
time-averaged VHE energy spectrum is well characterized by a power law model.
The broad-band light curve, including the available multiwavelength data, as
well as the VHE data gathered with H.E.S.S. will be presented.
