  We report the likely detection of gamma-ray emission from the northeast shell
region of the historical supernova remnant (SNR) SN 1006. Having analyzed 7
years of Fermi LAT Pass 8 data for the region of SN 1006, we found a GeV
gamma-ray source detected with 4 sigma significance. Both the position and
spectrum of the source match those of HESS J1504-418 respectively, which is TeV
emission from SN 1006. Considering the source as the GeV gamma-ray counterpart
to SN~1006, the broadband spectral energy distribution is found to be
approximately consistent with the leptonic scenario that has been proposed for
the TeV emission from the SNR. Our result has likely confirmed the previous
study of the SNRs with TeV shell-like morphology: SN 1006 is one of them
sharing very similar peak luminosity and spectral shape.
