The galaxy presents a discernible disk-like structure, viewed at an angle significantly offset from edge-on. The disk exhibits a spiral arm morphology, although the arms appear somewhat flocculent and not tightly wound. There is a noticeable central bulge, but it does not dominate the overall structure. A bar-like feature is present, running through the central region of the galaxy. The galaxy displays evidence of star formation, indicated by a blue hue and the presence of brighter knots within the spiral arms. No significant tidal features or signs of recent major mergers are immediately apparent, though some minor disturbances cannot be ruled out. The galaxy appears relatively isolated within its immediate environment.
