The galaxy presents as a spiral type, observed at a moderate redshift. It exhibits a prominent, but not dominant, central bulge that is yellow-orange in color, suggesting a population of older stars. The spiral arms are well-defined and appear to be winding loosely, with a predominantly two-arm structure. Patches of blue color are visible within the arms, indicative of on-going star formation. There is no clear evidence of a strong bar structure. Minor distortions appear to be present in the outer arms, which suggest possible minor gravitational interactions.
