The observed galaxy presents a distinct spiral morphology, viewed approximately face-on. The central bulge appears relatively prominent, exhibiting a moderate size compared to the overall galactic disk. Two well-defined spiral arms emanate from the galactic core, exhibiting a somewhat tightly wound structure. Flocculent features are visible along the arms. These features contribute to the overall luminosity and suggest ongoing star formation. No distinct bar structure is readily apparent, but it is possible a faint one is present. The galactic disk appears largely undisturbed, with no major signs of an ongoing merger.
