  We report on the closest view of a coronal mass ejection observed by the
Parker Solar Probe (PSP)/Wide-field Imager for {Parker} Solar PRobe (WISPR)
instrument on September 05, 2022, when PSP was traversing from a distance of
15.3~to~13.5~R$_\odot$ from the Sun. The CME leading edge and an arc-shaped
{\emph{concave-up} structure near the core} was tracked in WISPR~field of view
using the polar coordinate system, for the first time. Using the impact
distance on Thomson surface, we measured average speeds of CME leading edge and
concave-up structure as $\approx$2500~$\pm$~270\,km\,s$^{-1}$ and
$\approx$400~$\pm$~70\,km\,s$^{-1}$ with a deceleration of
$\approx$20~m~s$^{-2}$ for the later. {The use of the plane-of-sky approach
yielded an unrealistic speed of more than three times of this estimate.} We
also used single viewpoint STEREO/COR-2A images to fit the Graduated
Cylindrical Shell (GCS) model to the CME while incorporating the source region
location from EUI of Solar Orbiter and estimated a 3D speed of
$\approx$2700\,km\,s$^{-1}$. We conclude that this CME exhibits the highest
speed during the ascending phase of solar cycle 25. This places it in the
category of extreme speed CMEs, which account for only 0.15\% of all CMEs
listed in the CDAW CME catalog.
