  On 2018 November 5, about 24 hours before the first close perihelion passage
of Parker Solar Probe (PSP), a coronal mass ejection (CME) entered the field of
view of the inner detector of the Wide-field Imager for Solar PRobe (WISPR)
instrument onboard PSP, with the northward component of its trajectory carrying
the leading edge of the CME off the top edge of the detector about four hours
after its first appearance. We connect this event to a very small jet-like
transient observed from 1 au by coronagraphs on both the SOlar and Heliospheric
Observatory (SOHO) and the A component of the Solar TErrestrial RElations
Observatory mission (STEREO-A). This allows us to make the first
three-dimensional reconstruction of a CME structure considering both
observations made very close to the Sun and images from two observatories at 1
au. The CME may be small and jet-like as viewed from 1 au, but the close-in
vantage point of PSP/WISPR demonstrates that it is not intrinsically jet-like,
but instead has a structure consistent with a flux rope morphology. Based on
its appearance in the SOHO and STEREO-A images, the event belongs in the
"streamer blob" class of transients, but its kinematic behavior is very
unusual, with a more impulsive acceleration than previously studied blobs.
