The galaxy exhibits a clear spiral structure, although the arms are tightly wound and somewhat flocculent in appearance. The central bulge appears relatively prominent and luminous, suggesting a significant population of older stars. The disk component shows a bluer hue, indicative of ongoing star formation. There is a slight indication of asymmetry in the spiral arm structure. The galaxy is relatively well-defined, with a relatively smooth overall light distribution, suggesting a late-type spiral galaxy. The overall color suggests a relatively mature stellar population with ongoing star formation.
