The galaxy presents as a spiral type, exhibiting a prominent disk structure. There is evidence of distinct spiral arms emanating from the central region. The arms appear to be moderately wound, with a predominantly two-arm structure. The central bulge appears moderate in size relative to the disk, with a concentration of light towards the nucleus. There is a suggestion of a bar-like feature spanning the central region, but it is not strongly defined. The disk itself appears relatively undisturbed, showing no signs of major mergers, although a minor disturbance is possible. The blue tint of the disk suggests ongoing star formation.
