Observations

We only have low resolution images ( FWHM) made at 20 cm (A-array), 6 cm (B-array) and 2 cm (C-array). Additional 90 cm data is also present, but can only be used as a fluxmeasurement. Because this object is so large (more than 50 arcsec) the map shows a tiny bit of structure (the galaxy is slightly elongated instead of circular shaped).