The galaxy presents as a spiral galaxy with a moderate bulge. Traces of spiral arm structure are visible, extending from the central region, though the arms appear somewhat flocculent, without well-defined edges. The galaxy's light profile suggests a relatively high mass. The galaxy appears to be in a relatively undisturbed state with no obvious signs of a major merger, though there are indications of a minor disturbance in the structure, or perhaps an ongoing minor merger event. Star formation is ongoing, as evidenced by bluer regions, though it appears at a moderate rate. There is no indication of the presence of a strong bar structure in the galaxy's center. Overall, the galaxy exhibits characteristics consistent with a normal, relatively massive spiral galaxy with ongoing, moderate star formation.
