  We combined photographic, photoelectric and CCD observations of the nova-like
variable V380 Oph to get a light curve spanning the time range of 40 years.
While the typical high-state brightness of V380 Oph was R~14.5, two
low-brightness episodes identified in 1979 (B_pg~17.5) and 2015 (R~19) confirm
its classification as a VY Scl-type "anti-dwarf nova". The Fourier period
analysis of photoelectric and CCD V and B observations obtained in 2002-16
revealed the presence of two periods 0.148167d and 4.287d, that may be
associated with negative superhumps and disc precession. We also compared
measurements obtained with the iris micro-photometer and flatbed scanner at the
same plates and found an agreement within the expected accuracy of photographic
photometry.
