The object appears to be a spiral galaxy at an approximate redshift of 0.29. The galaxy displays a distinct disk structure with clear spiral arms. The spiral arms are tightly wound. The galaxy has two arms. There appears to be a bulge. The central bulge looks moderate in size. There is no evidence of a strong bar feature. The light distribution suggests ongoing star formation activity within the arms. There does not appear to be any major merging or disturbances in the galaxy. The estimated size of the galaxy is a median radius of approximately 9.3 kpc.
