The galaxy presents a disk-like structure with evident spiral arms. The arms appear to be relatively tightly wound around a central bulge. This bulge displays a moderate size relative to the overall galactic disk. There is no clear bar structure visible within the bulge region. The spiral arms exhibit a predominantly two-armed structure with hints of possible secondary arms. The overall appearance is somewhat disturbed, suggesting possible minor interaction or internal dynamical processes. The lack of a dominant bulge suggests it is not an elliptical galaxy.
