The galaxy presents as a spiral type, exhibiting a dominant disk structure. The spiral arms are visible and well-defined, originating from a central bulge that appears moderate in size. The arms are traced by regions of likely star formation. There is no strong evidence for a prominent bar feature. The overall color is slightly blue, suggesting a reasonably high rate of recent or ongoing star formation. The galaxy is likely relatively undisturbed, showing no significant signs of major mergers, although minor disturbances cannot be ruled out. The galaxy does not appear to be viewed edge-on.
