The galaxy appears to be a spiral galaxy, observed at a redshift of approximately 0.217. Its morphology exhibits prominent spiral arms with an estimated median of three arms. The winding of these arms appears to be medium, neither tightly wound nor exceptionally loose. The central bulge appears to be of moderate size, contributing significantly to the overall luminosity of the galaxy. There is no apparent bar structure visible within the central region. The disk is viewed face-on. There is an indication of some minor interaction or disturbance in the galaxy's morphology. Star formation activity is present, as evidenced by its blue luminosity.
