This galaxy appears to be a spiral type, exhibiting a prominent central bulge and a disk component. The bulge displays a yellowish hue, suggesting an older stellar population. Spiral arms are faintly visible, and appear somewhat flocculent and ill-defined, indicating a lack of grand design structure. The galaxy's disk presents a bluer color, indicative of ongoing star formation. There is morphological evidence of potential interaction or merger activity, specifically disturbance in the spiral arm structure. A bar feature is suspected, bisecting the bulge, but it is weak. The galaxy is seen close to face-on.
