  We present results from a first analysis of optical data on G 69.4+2.4
obtained with the 0.3 m and 1.3 m telescopes at Skinakas Observatory.
Filamentary emission is detected in the [OIII] 5007 A and Halpha+[NII] images
oriented in the south-west, north-east direction. The Halpha+[NII] images
reveal a complex network of filaments, while the [OIII] images show a single
filament. Low resolution spectra were also obtained which identify the observed
emission as emission from shock heated gas.
