The galaxy presents as a spiral type, characterized by a prominent, though somewhat indistinct, central bulge. Two well-defined spiral arms emanate from this central region, displaying a moderate winding. Star forming regions are evident within the spiral arms with bluish hue. The disk component appears significant in size.  Overall structure suggests a relatively unperturbed morphology, showing no obvious signs of major interaction or merging events, although there is some apparent disturbance in the lower arm. There is a hint of a bar structure in the central region, though its morphology is difficult to assess.
