This galaxy presents as a face-on spiral. Two clearly defined spiral arms dominate its structure. These arms appear loosely wound, extending outwards from a central bulge region. The bulge is relatively small, making up a moderate proportion of the galaxy’s total light.

The color distribution suggests ongoing star formation, particularly within the spiral arms, indicated by the presence of bluer regions. There appears to be a bar-like feature traversing the central region of the galaxy, possibly a weak or nascent bar structure. There are no obvious signs of significant tidal disturbances or interactions with other galaxies, although a minor perturbation cannot be ruled out.
