The galaxy exhibits a clear spiral structure. The arms are well-defined and extend from a central, moderately sized bulge. The winding of the spiral arms appears relatively tight. Dust lanes are subtly visible within the arms, contributing to a somewhat flocculent texture. There is a possible weak bar structure present. No significant signs of tidal disturbances or major mergers are apparent. The overall color suggests a relatively high rate of star formation, particularly within the spiral arms. The luminosity profile appears consistent with a late-type spiral galaxy.
