The galaxy presents as a face-on or nearly face-on spiral galaxy, displaying a prominent disk structure with a noticeable central bulge. Spiral arms are visible and appear loosely wound. A small disturbance can be seen in the disk of the galaxy, indicating the possibility of a minor gravitational interaction or merger event.

The central bulge exhibits a bright, yellowish hue suggesting a population of older stars. Patches of blue color, especially in the spiral arms, indicate regions of active star formation. The general color distribution indicates ongoing star formation in the outer regions of the disk.
