Supernova Remnants (SNRs) play an essential role in galaxies, enriching the Interstellar Medium (ISM) producing a significant impact on their structure and physical properties. The Honeycomb Nebula (MC SNRJ0535–6918) is one of the most peculiar SNRs in the Large Magellanic Cloud (LMC) – just a few arcminutes south-east of the well-known SN 1987A. It was discovered in the X-ray band in the ROSAT survey. Alsaberi et al. present the first and deepest ATCA radio continuum images of the Honeycomb Nebula at 2000 and 5500 MHz solely from archival data. They find an average radio spectral index for the remnant of −0.8. Polarisation maps at 5500 MHz reveal an average fractional polarisation of 25 ± 5% with a maximum value of 95 ± 16%. They estimate the equipartition field for Honeycomb Nebula of 48 ± 5 µG. Finally, using 21cm HI data, they support the idea that the Honeycomb Nebula exploded inside a low-density wind cavity. The iamge above shows the ATCA intensity image of the Honeycomb Nebula at 5500 MHz. The ellipse at the bottom left corner represent a synthesised beam of 1.3×1.2 arcsec ² .