  We report the discovery of 2010 GB$_{174}$, a likely new member of the Inner
Oort Cloud (IOC). 2010 GB$_{174}$ is one of 91 Trans Neptunian Objects (TNOs)
and Centaurs discovered in a 76 deg$^2$ contiguous region imaged as part of the
Next Generation Virgo Cluster Survey (NGVS) --- a moderate ecliptic latitude
survey reaching a mean limiting magnitude of $g^\prime \simeq 25.5$ --- using
MegaPrime on the 3.6m Canada France Hawaii Telescope. 2010 GB$_{174}$ is found
to have an orbit with semi-major axis $a\simeq350.8$ AU, inclination $i \simeq
21.6^\circ$ and pericentre $q\sim48.5$ AU. This is the second largest
perihelion distance among known solar system objects. Based on the sky coverage
and depth of the NGVS, we estimate the number of IOC members with sizes larger
than 300 km ($H_V \le 6.2$ mag) to be $\simeq 11\,000$. A comparison of the
detection rate from the NGVS and the PDSSS (a characterized survey that
`re-discovered' the IOC object Sedna) gives, for an assumed a power-law LF for
IOC objects, a slope of $\alpha \simeq 0.7 \pm 0.2$, with only two detections
in this region this slope estimate is highly uncertain.
