2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/7246We present time-resolved CCD photometry of V2275 Cyg 790 days after the nova outburst. The data show a 20% peak-to-peak oscillation with a period of 24 minutes. The period appears stable over the two nights of observation, but QPO can not be ruled out.3 pages, 3 postscript figures, uses ibvs2.sty, to be published in IBVSAstrophysicstext