It is a Be star; a rapidly rotating star that is hosting a circumstellar disk of hot, decreted gas. It is a photometrically variable Be star, having a brightness that ranges from 4.4 down to 4.51 in visual magnitude, and has been classified as a Gamma Cassiopeiae variable.
As a Be star, it is rapidly rotating and has a circumstellar disk of hot, condensed gas. The star displays photometric variability, with brightness varying from 4.4 to 4.51 in visual magnitude, and is categorized as a Gamma Cassiopeiae variable.