The SIMBAD database lists UGC11861 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.[4] In addition, the galaxy contains two broad spiral arms wrapping around its central region.[5]
^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.
^"SN1995ag". 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.
^"SN1997db". 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.
^"SN2011dm". Transient Name Server. IAU. Retrieved 19 August 2024.