We present supporting evidence for the first association of a Fermi source , 3FGLJ1330.0-3818 , with the FR 0 radio galaxy Tol1326-379 .
FR 0s represent the majority of the local radio loud AGN population but their nature is still unclear .
They share the same properties of FR Is from the point of view of the nuclear and host properties , but they show a large deficit of extended radio emission .
Here we show that FR 0s can emit photons at very high energies .
Tol1326-379 has a GeV luminosity of L _ { > 1 ~ { } { GeV } } \sim 2 \times 10 ^ { 42 } erg s ^ { -1 } , typical of FR Is , but with a steeper \gamma -ray spectrum ( \Gamma = 2.78 \pm 0.14 ) .
This could be related to the intrinsic jet properties but also to a different viewing angle .