  The analysis of photometrical observations of comet 29P/Schwassmann-Wachmann
1 is presented. The broadband observations were carried out for 15 nights from
2012 to 2019 at the Lisnyky observational station of Taras Shevchenko National
University of Kyiv. Apparent magnitudes and dust productivity level $Af\rho$ in
filter R were calculated. Middle and height dust activity of the comet is
characterized by parameter $Af\rho$ which varied from 1246 to 17563 cm during
all periods of observation. Based on the morphological analysis, four jet-like
structures were detected in the coma on almost all dates. Using the geometrical
model for the jet structure interpretation during all observation sets, we
obtained following results: the nucleus rotation periodof 57\pm2 days, the
rotational axis orientation, the locations of active regions for four jet-like
structures within a narrow belt near the equator.
