The galaxy exhibits a distinct spiral structure. Though somewhat ill-defined, there are indications of spiral arms emanating from a brighter central region. These arms appear flocculent rather than grand design. Dust lanes are likely present within the spiral arms, contributing to the patchy appearance.

The galactic disk appears face-on. A bulge is evident, though it is neither dominant nor particularly large in relation to the rest of the galaxy, perhaps small to moderate in size. A weak bar structure may be present in the central region. The overall color is skewed toward the blue end of the spectrum, suggesting a population of younger, hotter stars, and active star formation within the galaxy, though the blue light may simply be from increased dust scattering. There are no signs of significant tidal disturbances or ongoing major mergers.
