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The SIMBAD database lists UGC 11861 an active galaxy nucleus candidate, i.e. it has a compact region at the center that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars. In addition, the galaxy contains two broad spiral arms wrapping around its central region.
Mueller, J.; Griffith, D.; Brewer, C.; Mendenhall, J. D.; Reid, I. N.; Gizis, J. (1995). "Supernova 1995ag in UGC 11861". International Astronomical Union Circular (6244): 1. Bibcode:1995IAUC.6244....1M.
"SN 1995ag". Transient Name Server. IAU. Retrieved 19 August 2024.
Schwartz, M.; Offutt, W.; Filippenko, A. V.; Leonard, D. C.; Gilbert, A. M. (1997). "Supernova 1997db in UGC 11861". International Astronomical Union Circular (6711): 2. Bibcode:1997IAUC.6711....2O.
"SN 1997db". Transient Name Server. IAU. Retrieved 19 August 2024.
Kandrashoff, M.; Kelly, J.; Cenko, S. B.; Li, W.; Filippenko, A. V. (2011). "Supernova 2011dm in UGC 11861 = PSN J21564159+7317489". Central Bureau Electronic Telegrams. 2745: 1. Bibcode:2011CBET.2745....1K.
"SN 2011dm". Transient Name Server. IAU. Retrieved 19 August 2024.