The galaxy presents a discernible disk structure, exhibiting a predominantly face-on orientation with slight inclination. Evident spiral arms are visible, extending from the galactic center. A weak bar structure is suspected within the central region. The bulge appears to be moderate in size relative to the disk, with a noticeable, though not dominant, presence.

The galaxy displays a relatively smooth appearance, with some indications of internal features, yet lacking major disturbances or significant merging activity. The overall color is a pale blue, suggesting the presence of ongoing star formation.
