We will post a light curve on the Bellatrix Observatory's website as soon as possible. So, this star is a new member of the SU UMa class. The campaign promoter is you, Gianluca Masi, and we Kyoto team will surely join soon. We will make a necessary set-up for a web page for presenting the results. The quiescent magnitude was reported as 18, but the V-band photometry at the Ouda station set an upper limit of 18.3.
Further observations are strongly encouraged.