The galaxy presents as a face-on spiral, though the spiral arms are somewhat difficult to discern. The central bulge is moderately sized and appears yellowish-orange, suggesting an older stellar population. The arms exhibit bluer tones, indicative of ongoing star formation. There may be a faint bar feature across the center. The disk component appears to be the dominant feature of the galaxy, with spiral arms that can be seen as clumpy regions, characteristic of areas of higher density of stars and ionized gas. There are no obvious signs of major mergers or significant tidal disturbances. The galaxy exhibits a smooth overall morphology with subtle features. The dust lanes are hard to see because of the low resolution of this image.
