The galaxy presents as a spiral with a notable disk structure. High likelihood of strong spiral arms. There appears to be a prominent central bulge with a yellow and orange hue, suggesting an older stellar population. Disk structure seems to be more prominent on one side of the bulge than the other, suggesting an angle of observation that is slightly off from being perfectly face-on. No indication of significant tidal disturbances or ongoing major merger events. There is no dust lane visible. No obvious indications of a strong central bar.
