A search of dust structures nearby the pulsar J0302+2252 in IRIS, AKARI, and WISE surveys were performed using Skyview Observatory (http://skyview.gsfc.nasa.gov). The physical properties have been studied at 60µm & 100µm in the IRIS survey, 90µm & 140µm in the AKARI survey, and 12µm & 22µm in the WISE survey at right ascension (R.A.) (J2000)=03h 02m 31.99s and Declination (Decl.) (J2000)=+ 220 52m 12.10s . In this work, we have studied the physical properties such as Dust color temperature, Planck’s function, Visual extinction, and Mass profile of the dust using the data reduction software ALADIN v11. The dust color temperature is found to be 22.271 ±  0.261K in IRIS, 22.343 ±  0.939 K in AKARI, and 278.74 ±  0.067 K in WISE. Also, the dust mass is found to be 2.286 ×  1027 kg (1.149 ×  10-3 M⊙  ) in IRIS, 8.800 × 1026 kg (0.416×  10-3 M⊙  ) in AKARI and 5.220 × 1025 kg (0.026 × 10-3 M⊙  ) in WISE. The average visual extinction is found to be 1.372 × 10-13 mag. In IRIS, 4.970 × 10-14 mag. In AKARI and 1.673 × 10-15 mag. In WISE. The dust color temperature and dust mass distribution show a very good agreement with Gaussian. The Contour plots of dust color temperature and dust mass show inverse relation between them in all three bands IRIS, AKARI, and WISE.