This is an evolved red giant star with a stellar classification of M2 IIIa.[4] It is a semiregular variable star of subtype SRB with a magnitude that ranges from a high of 4.80 down to 5.00.[6] The measured angular diameter of this star, after correcting for limb darkening, is {{Val|4.79|0.34|u=mas}}.[25] At its estimated distance, this yields a physical size of 88 times the radius of the Sun.[12]
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1 {{citation | display-authors=1 | title=Rotational velocities of the giants in symbiotic stars - III. Evidence of fast rotation in S-type symbiotics | last1=Zamanov | first1=R. K. | last2=Bode | first2=M. F. | last3=Melo | first3=C. H. F. | last4=Stateva | first4=I. K. | last5=Bachev | first5=R. | last6=Gomboc | first6=A. | last7=Konstantinova-Antova | first7=R. | last8=Stoyanov | first8=K. A. | journal=Monthly Notices of the Royal Astronomical Society | volume=390 | issue=1 | pages=377–382 | date=October 2008 | doi=10.1111/j.1365-2966.2008.13751.x | bibcode=2008MNRAS.390..377Z | arxiv=0807.3817 | postscript=. }}
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1 {{citation | display-authors=1 | last1=Richichi | first1=A. | last2=Percheron | first2=I. | last3=Khristoforova | first3=M. | title=CHARM2: An updated Catalog of High Angular Resolution Measurements | journal=Astronomy and Astrophysics | postscript=. | volume=431 | issue=2 | pages=773–777 | date=February 2005 | doi=10.1051/0004-6361:20042039 | bibcode=2005A&A...431..773R }}
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*) is given by::
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