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The observations revealed an optical source with $r'$ = 23.33$\\pm$0.02 and $i'$=23.08$\\pm$0.02, whose position coincides with the pulsar radio position. By comparing the source colour and magnitudes with the white dwarf cooling predictions, we found that it likely represents a He or CO-core white dwarf and estimated its mass of 0.52$^{+0.25}_{-0.19}$ M$_{\\odot}$ and effective temperature of 6300$^{+1000}_{-800}$ K. 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