The galaxy presents as a spiral, nearly edge-on. It exhibits tightly wound spiral arms, and a central bulge that appears moderate in size.  Dust lanes are visible within the disk, contributing to the obscuration. The disk shows signs of disturbance, possibly due to a minor interaction or internal dynamics.  Overall, the galaxy appears relatively blue, suggesting ongoing star formation. The ellipticity is high. There is a weak or absent bar present in the center.
