Аннотация:We present new photometric data, taken at the Crimean Laboratory of Sternberg Astronomical Institute and University of Dallas, on the suspected intermediate polar V795 Her. Photometry reveals a period of 0.115487 days. This period, when compared with past observations, shows a slight modulation and even a complete disappearance in mid-1990. Light curves of V795 Her are also shown to demonstrate some superhump activity. Superhumps as the possible result of accretion disk precession are discussed.