The data analysis on a wider time interval to find a possible weak signal or to establish the limit on the neutrino emission is in progress. Comparison with the H-band image of Masetti et al. This is in the outskirts of a spiral arm, 0.9 arcsec west of the apparent nucleus of a face-on spiral galaxy. The galaxy appears to be of type Sc, possibly with a weak bar. The image size is 2048 x 2048 pixels, and the image scale is 0.0254 arcseconds per pixel.
North is up and East is to the left.
The total exposure time is 8851 seconds. Observations have been carried out under seeing conditions of 0.6-0.7 arcsec. Considering the V-band aperture magnitude obtained by Holland et al. This message can be cited.