The galaxy presents as a spiral type, observed at an angle that is noticeably offset from face-on. Two spiral arms are distinctly visible, tracing a path from the central region outward. These arms exhibit a moderate winding, neither tightly coiled nor completely open. A bar-like structure is present within the central region of the galaxy, contributing to its overall spiral morphology.

The central bulge appears moderate in size relative to the galactic disk. There is no obvious ongoing major merger, but some minor disturbances may be present.
