  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 $(1.8\pm0.7)\times10^{-6}$ 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
$1.1\times10^{-7}$ ph cm$^{-2}$ s$^{-1}$ and $5.2\times10^{-10}$ 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
$(13.56\pm0.02)\times10^{-8}$ ph cm$^{-2}$ s$^{-1}$ that is highly variable on
monthly timescales. We associate this emission with the known quasar 87GB
215950.2+503417.
