This galaxy exhibits a pronounced disk structure, viewed at a slight angle from face-on. Distinct spiral arms are visible, appearing somewhat tightly wound around the galactic center. The central bulge appears moderately sized, contributing significantly to the overall luminosity. Evidence suggests the presence of a bar feature crossing the central region, potentially altering the structure of the spiral arms. The galaxy shows color variations indicative of active star formation regions within the spiral arms, alongside older stellar populations near the bulge. There is no strong evidence of major ongoing mergers, but some minor disturbances can be observed. The galaxy is estimated to be about 9 kiloparsecs in radius, given its distance based on its redshift.
