  We report a possible detection of TeV gamma-rays from the Galactic Center by
the Whipple 10m gamma-ray telescope. Twenty-six hours of data were taken over
an extended period from 1995 through 2003 resulting in a total significance of
3.7 standard deviations. The measured excess corresponds to an integral flux of
\Flux above an energy of $2.8 \mathrm{TeV}$, roughly 40% of the flux from the
Crab Nebula at this energy. The 95% confidence region has an angular extent of
about 15 arcmin and includes the position of Sgr A*. The detection is
consistent with a point source and shows no evidence for variability.
