The galaxy presents as a spiral galaxy, exhibiting a prominent disk structure. It has a generally elliptical shape, with a noticeable bulge at its center. The spiral arms are loosely wound and somewhat flocculent, indicating differential rotation within the galactic disk. The central bulge appears to be a significant fraction of the overall galaxy size. There is evidence of a possible bar structure traversing the central region. The galaxy exhibits a relatively smooth appearance, with some localized areas of increased light intensity. The observed color gradients across the galaxy suggest varying stellar populations and dust distribution, with bluer regions potentially indicating areas of active star formation and younger stars. There is no obvious signs of recent major merger events.
