The object is a spiral galaxy with a redshift indicative of a relatively nearby system. The galaxy exhibits a distinct disk structure with prominent spiral arms. These arms appear somewhat tightly wound near the central bulge, becoming more diffuse and loosely defined further out. Two main spiral arms appear to dominate the overall structure. A bar structure is also present. The central bulge is not very dominant. Patches of bluer light are observed along the spiral arms, suggesting regions of active star formation. There are no major signs of mergers, however some disturbances are present. The galaxy's disk is oriented close to face-on with only a slight inclination relative to our line of sight.
