The galaxy presents as a relatively large, luminous system, likely a spiral or lenticular galaxy viewed at a slight inclination. A bright, yellowish central bulge dominates the core, suggesting a significant population of older stars. Fainter spiral arms or a disk structure surround the bulge, displaying a bluer hue, indicative of ongoing star formation. However, the disk exhibits a patchy and somewhat disturbed morphology. There is some evidence of minor disturbance, with asymmetry present in the outer regions of the disk. The color gradient from the center to the outer regions is apparent, transitioning from yellow to a bluer shade, indicative of younger star formation. The galaxy is moderately distant, with an estimated size exceeding 10 kiloparsecs.
