The galaxy presents as a spiral type, observed at a moderate inclination. The bulge appears prominent, though not dominant, exhibiting a moderate degree of concentration. Faint spiral arm structures extend from the central bulge, displaying a relatively open morphology. The disk exhibits a non-negligible amount of patchy star formation activity, indicated by the presence of bluer regions within the spiral arms. There is a suggestion of a bar feature crossing the bulge. The galaxy exhibits a smooth outer halo, with the disk appearing to be warped.
