  The Seyfert galaxy NGC 1275 is the central, dominant galaxy in the Perseus
cluster of galaxies. NGC1275 is known as a powerful source of radio and X-ray
emission. The well-known extragalactic object NGC 1275 has been observed by the
SHALON high-altitude mirror Cherenkov telescopes within the framework of
long-term studies of metagalactic gamma-ray sources. In 1996, the SHALON
observations revealed a new metagalactic source of very high energy gamma-ray
emission coincident in its coordinates with the galaxy NGC 1275. Having
analyzed the SHALON data, we have determined such characteristics of NGC 1275
as the spectral energy distributions and images at energies >800 GeV for the
first time. The results obtained at high and very high energies are needed for
understanding the emission generation processes in an entire wide energy range.
