NSV 2798 = GSC 1325-1771, at 6 03 11.9 +22 03 30 (2000). As far as I know there is no broadband photometry (BVRI) of any kind in the region of this star. You might consider using some of the brighter nearby Tycho-2 stars for a reasonable zero-point calibration for B and V. Be sure to correct the Tycho data to the standard system, and avoid stars with errors of 0.03 mag. in either B or V. Another option is to use stars in the $B(Bearbopen(B $BclusteMessie35(B $Bforeference.(B $BTheris(B $Brecent(B $BUBVI(B $Bphotometry(B $Bfothclusteby(B $BSung(B $BanBessel(199MNRA306,361)(B $BData(B $Bancharts(B $Bfothclustecabe(B $Bobtained(B $Bfrom(B $BJean-ClaudMermilliod's(B $Bopen(B $Bclustedatabase(B $Bstarting(B $Bat(B $Bhttp://obswww.unige.ch/webda/navigation.html(B $B\Brian(B $B(B