The galaxy presents as a somewhat face-on spiral, though the disk structure is not sharply defined. A bright, prominent central bulge dominates the galaxy's core, displaying a yellowish-orange hue, suggesting an older stellar population. Surrounding the bulge, the spiral arms exhibit a bluer tint, indicative of more recent star formation. The arms are not tightly wound, appearing rather flocculent and less distinct. There's some evidence of dust lanes, particularly on the left side of the galaxy, appearing as dark patches against the brighter regions. The overall morphology suggests a galaxy undergoing moderate star formation, with a significant population of older stars concentrated in the bulge. There appears to be some minor irregularity in the shape of the disk, possibly hinting at past interactions or disturbances.
