The galaxy presents as a spiral type, displaying discernible arm structures. These spiral arms are somewhat patchy and not as tightly wound. The disk appears to be oriented close to face-on with a prominent central bulge. The bulge appears moderately sized, and the galaxy exhibits a yellowish hue, possibly indicating a population of older stars and a moderate level of on-going star formation. There is also evidence of some disruption or irregularity in the disk, which could be indicative of a minor or major disturbance.
