We report an updated analysis of the gamma-ray source AGL J2241+4454 that was detected as a brief two-day flare in 2010 by the AGILE satellite . The high-energy emission of AGL J2241+4454 has been attributed to the binary system HD 215227 , which consists of a Be star being orbited by a black hole making it the first known Be-black hole binary system . We have analyzed the AGILE data and find a gamma-ray flux of ( 1.8 \pm 0.7 ) \times 10 ^ { -6 } ph cm ^ { -2 } s ^ { -1 } , in agreement with the initial report . Additionally , we examined data from the Fermi LAT over several time intervals including the two day flare , the folded orbital phase , and the entire mission ( \sim 6-years ) . We do not detect AGL J2241+4454 over any of these time periods with Fermi and find upper limits of 1.1 \times 10 ^ { -7 } ph cm ^ { -2 } s ^ { -1 } and 5.2 \times 10 ^ { -10 } ph cm ^ { -2 } s ^ { -1 } for the flare and the full mission , respectively . We conclude that the HD 215227 Be-black hole binary is not a true gamma-ray binary as previous speculated . While analyzing the Fermi data of the AGL J2241+4454 region , we discovered a previously unknown gamma-ray source with average flux of ( 13.56 \pm 0.02 ) \times 10 ^ { -8 } ph cm ^ { -2 } s ^ { -1 } that is highly variable on monthly timescales . We associate this emission with the known quasar 87GB 215950.2+503417 .