  We present a detailed radio-continuum study on Australia Telescope Compact
Array (ATCA) observations of Large Magellanic Cloud (LMC) supernova remnant
(SNR), MCSNR J0536-7038. This Type Ia SNR follows a horseshoe morphology, with
a size 32 pc $\times$ 32 pc (1-pc uncertainty in each direction). It exhibits a
radio spectrum $\alpha=-0.52\pm0.07$ between $\lambda = 73$ and 6 cm. We report
detections of regions showing moderately high fractional polarisation at 6 cm,
with a peak value of 71$\pm$25% and a mean fractional polarisation of
35$\pm$8%. We also estimate an average rotation measure across the remnant of
-237 rad m$^{-2}$. The intrinsic magnetic field appears to be uniformly
distributed, extending in the direction of the two brightened limbs of the
remnant.

High Energy Astrophysical Phenomena;Astrophysics of Galaxies