Context : The Supernova Remnants ( SNRs ) known in the Large Magellanic Cloud ( LMC ) show a variety of morphological structures in the different wavelength bands .
This variety is the product of the conditions in the surrounding medium with which the remnant interacts and the inherent circumstances of the supernova event itself .

Aims : This paper performs a multi-frequency study of the LMC SNR J0530–7007 by combining Australia Telescope Compact Array ( ATCA ) , Molonglo Observatory Synthesis Telescope ( MOST ) , Röntgensatellit ( ROSAT ) and Magellanic Clouds Emission Line Survey ( MCELS ) observations .

Methods : We analysed radio-continuum , X-ray and optical data and present a multi-wavelength morphological study of LMC SNR J0530–7007 .

Results : We find that this object has a shell-type morphology with a size of 215″ \times 180″ ( 52 pc \times 44 pc ) ; a radio spectral index ( \alpha = -0.85 \pm 0.13 ) ; with [ S ii ] /H { \alpha } > 0.4 in the optical ; and the presence of non-thermal radio and X-ray emission .

Conclusions : We confirmed this object as a bona-fide shell-type SNR which is probably a result of a Type Ia supernova .