Dear Colleagues, we performed photometric observations until few minutes ago of this star, getting a good run, about 3.7 hours long, under very good sky conditions. Preliminary analysis follows. The resulting lightcurve (as always, very impressive) shows that the features previously reported are still strong. We observed three main maxima and two eclipses. The shape os these ecplises is quite sharp. The secondary maxima are very interesting. As previously reported by G. Masi, they continue to be of two different kinds. We note that the modulation reduced its amplitude to 0.3 magnitudes. During the run, the star faded of about 0.05 magnitudes. Later today, we will providing a light curve. Follow-up is urgently needed. Gianluca Masi, Franco Mallia