The galaxy presents as a face-on spiral galaxy with a prominent bulge. The central bulge appears bright and nearly spherical in shape, indicating a high concentration of stars. Faint spiral arms emanate from the bulge, displaying a relatively flocculent structure, as they are loosely wound and less defined. The color profile exhibits a yellow-white hue in the central region, transitioning to a bluer tint towards the outer disk, suggesting ongoing star formation. There is a possible slight disturbance on one side of the disc. Overall, the galaxy appears as an intermediate-mass spiral galaxy, possibly undergoing moderate star formation activity within its disk and spiral arms.
