  We present results from a campaign of simultaneous X-ray and optical
observations of X1254-690 conducted using the Rossi X-ray Timing Explorer and
the CTIO 1.5m telescope. We find that the usually-observed deep X-ray dipping
is not seen during the times of our observations, with an upper limit of ~2% on
any X-ray orbital variation, and that the mean optical variability has declined
in amplitude from 0.40+-0.02 mag (in V) to 0.28+-0.01 mag. These findings
indicate that the vertical structure on the disk edge associated with the
impact point of the accretion stream has decreased in angular size from 17-25
degrees to <10 degrees, and support the suggestions of previous modeling work
that the bulge provides 35-40% of the contribution to the overall optical
modulation. The average optical and X-ray brightnesses are comparable to their
values during dipping episodes, indicating that the mean accretion rate and
disk radius remain unchanged.
