  We present the analysis of the planetary microlensing event
OGLE-2014-BLG-1760, which shows a strong light curve signal due to the presence
of a Jupiter mass-ratio planet. One unusual feature of this event is that the
source star is quite blue, with $V-I = 1.48\pm 0.08$. This is marginally
consistent with source star in the Galactic bulge, but it could possibly
indicate a young source star in the far side of the disk. Assuming a bulge
source, we perform a Bayesian analysis assuming a standard Galactic model, and
this indicates that the planetary system resides in or near the Galactic bulge
at $D_L = 6.9 \pm 1.1 $ kpc. It also indicates a host star mass of $M_* = 0.51
\pm 0.44 M_\odot$, a planet mass of $m_p = 180 \pm 110 M_\oplus$, and a
projected star-planet separation of $a_\perp = 1.7\pm 0.3\,$AU. The lens-source
relative proper motion is $\mu_{\rm rel} = 6.5\pm 1.1$ mas/yr. The lens (and
stellar host star) is predicted to be very faint, so it is most likely that it
can detected only when the lens and source stars are partially resolved. Due to
the relatively high relative proper motion, the lens and source will be
resolved to about $\sim46\,$mas in 6-8 years after the peak magnification. So,
by 2020 - 2022, we can hope to detect the lens star with deep, high resolution
images.
