The object appears to be a spiral galaxy exhibiting a disk-like structure with visible spiral arms. The arms are somewhat flocculent in nature and appear to be loosely wound. A central bulge is present; it appears small relative to the overall disk size and exhibits a yellowish hue, suggesting a population of older stars. The disk shows a bluer color profile, which is consistent with the presence of younger, hotter stars within the spiral arms. There are some visible dust lanes throughout the disk but they are not very prominent. Overall, the galaxy appears to be relatively undisturbed, without significant signs of major recent merging activity.
