The galaxy presents as a barred spiral with a moderately sized bulge relative to the disk. The spiral arms appear multi-armed and tightly wound close to the bulge region, then gradually open into a less defined morphology as they extend outwards. There is a slight asymmetry in the arm structure on one side, suggesting a potential minor gravitational interaction, or perhaps just a high rate of star formation.

The light distribution suggests a dominant disk component. The central bulge exhibits a yellow-white hue. The spiral arms present bluer colors indicative of active star formation. Overall, the galaxy appears well-defined, though the outer regions exhibit a lower surface brightness and are more difficult to discern clearly.
