  We have observed EY Draconis with the 24`` telescope of Konkoly Observatory
in Budapest for 64 nights. In the first obse rving season the star produced a
stable light curve for more than 60 rotation periods, however, the light curves
observe d in the next season and the spot modelling show clear evidence of the
evolution of the spotted stellar surface. The chan ges of the maximum
brightness level suggests the existence of a longer period of about 300 days,
which seems to be confir med by the ROTSE archival data.
