The UBV observations of a marginal contact system BX And obtained duri
ng 1987, 1989 and 1990 seasons at the Ankara University Observatory ar
e presented. Based on all available light curves of the system we stud
ied light curve variations, particularly at the extrema points. Time s
cale of the variations was found as short as a few cycles of the orbit
al revolution. Six new estimates of the minima times are given. Some i
ndications are found that the system might be detached or semi-detache
d.