The galaxy presents as a spiral galaxy, seen at a moderate inclination. The spiral arms are tightly wound and numerous, though difficult to resolve individually. A substantial bulge is apparent, comprising approximately half the galaxy's overall diameter. The bulge exhibits a smooth, yellowish hue, suggestive of an older stellar population. A bar structure seems to traverse the bulge, running horizontally through the major axis, though its presence is somewhat indistinct. The disk appears to be actively forming stars, with a bluer color indicative of younger, hotter stars. The morphology shows no indications of any recent major merger events, disturbances, or other galactic interactions.
