The galaxy appears to be a spiral galaxy, observed at a redshift of approximately 0.2. The structure is characterized by a prominent central bulge. Faint spiral arms emerge from the bulge. The arms appear somewhat tightly wound. The colour gradient suggests ongoing star formation within the disk, with bluer regions likely indicating areas of active star birth, contrasted against the older stellar populations in the bulge, which appear redder. The galaxy does not show evidence of a major ongoing merger, but a minor disturbance cannot be ruled out. There appears to be a weak bar structure visible in the centre of the galaxy. There may be two apparent spiral arms.