The galaxy presents as a spiral type, observed at an oblique angle to our line of sight. It exhibits a prominent, moderately sized central bulge, appearing yellowish, likely indicating an older stellar population. Fainter spiral arms emanate from the central region. The arms are moderately wound and somewhat diffuse, suggesting they are not sharply defined. Two spiral arms dominate. The overall structure appears generally undisturbed, showing no strong signs of major interactions or mergers. There is a hint of a bar-like structure, though it is not strongly pronounced.
