The object appears to be a spiral galaxy, observed at an inclination angle that is neither face-on nor edge-on. There is a central bulge visible with a yellowish hue, suggesting an older stellar population. Faint spiral arms are present. The arms appear somewhat flocculent, with less tightly wound morphology. There appear to be two main arms emanating from opposite sides of the bulge region. The overall color of the disk component is bluer than the bulge. No prominent features are indicative of strong tidal interactions or recent major mergers, although the possibility of minor disturbances cannot be ruled out.
