  The main aim of photometrical observations of the asteroid 3200 Phaethon was
searching for its low-level cometary activity (possible coma and/or dust tail)
in the pre-perihelion passage. We performed observational runs with telescopes
ranging from 0.61-m to 2-m and BVR color imaging. Three longer photometric
series were used for modeling of the 3D shape of Phaethon. The color indices
and size of the asteroid were estimated.
