The observed galaxy presents as a spiral galaxy with a moderate inclination relative to the line of sight. The galaxy exhibits a discernible central bulge which appears yellowish. Faint spiral arms extend outwards from the central bulge, indicating a grand design spiral structure. The arms appear somewhat tightly wound. Star formation is likely occurring within the arms, suggested by the presence of blue light. It appears that the galaxy is barred, though the bar structure itself seems relatively weak and difficult to precisely identify. No significant tidal disturbances or signs of a major merger are apparent in this imaging data. The central bulge may contain a weak active galactic nuclei.
