The galaxy presents as a spiral type, exhibiting prominent, well-defined spiral arms. The arms appear somewhat flocculent and extend outward from a bright central bulge. The bulge itself is moderately sized, displaying a smooth, concentrated luminosity profile, indicative of an older stellar population.

Dust lanes are visible within the spiral arms, obscuring some of the starlight and contributing to the observed patchy texture. Star formation is likely occurring within these arms as suggested by the slightly blueish tinge. The galaxy appears relatively undisturbed with no immediately obvious signs of a major merger event. The galactic disk is not perfectly edge-on, allowing for a clear view of the spiral structure. There is a weak suggestion of a bar-like structure.
