CCD photometry of the visual companion of the Cepheid FF Aql is presen
ted. The magnitude and colors of the companion are V=11.14 +/- 0.07 ma
g, B-V=0.60+/-0.05 mag, and V-R=0.39+/-0.04 mag. The separation is 6.'
'89+/-0.''18 and the position angle 143.9-degrees +/- 2-degrees. The c
ompanion is too bright and/or too red to be a Zero-Age Main-Sequence s
tar at the distance of the Cepheid with the observed color, whether th
e Cepheid is pulsating in the fundamental mode or the first overtone.
Only if the errors in the color are underestimated can the companion b
e a member of the FF Aql system. (Contamination by the Cepheid would m
ake the companion brighter and redder.) Positional measurements show a
pparent motion which is too large to be orbital motion. Thus, it is no
t likely that the 6'' companion is physically associated with the Ceph
eid FF Aql.