We present a radio and optical study of the double-double radio galaxy J1328+2752 based on new low-frequency GMRT observations and SDSS data . The radio data were used to investigate the morphology and to perform a spectral index analysis . In this source we find that the inner double is misaligned by \sim 30 ^ { \circ } from the axis of the outer diffuse structure . The SDSS spectrum shows that the central component has double-peaked line profiles with different emission strengths . The average velocity off-set of the two components is 235 \pm 10.5 km s ^ { -1 } . The misaligned radio morphology along with the double-peaked emission lines indicate that this source is a potential candidate binary supermassive black hole . This study further supports mergers as a possible explanation for repeated jet activity in radio sources .