The galaxy appears as a relatively face-on spiral, exhibiting a central bulge that dominates the overall light distribution. The bulge is smooth and appears to be composed of older stellar populations, indicated by its yellow-white hue. The galaxy displays a disk structure with hints of spiral arms, which extend outwards from the central bulge. These arms are bluer in color, suggesting ongoing star formation. The dust lanes are visible, silhouetted against the brighter stellar regions of the disk. The galaxy exhibits an overall flattened shape, with an elliptical outline.
