This galaxy presents as an elongated, disk-like structure, seen at a significant angle relative to our line of sight. There is a discernible bulge component that appears approximately spherical and exhibits a yellowish-orange hue, suggesting a population of older, cooler stars. The disk exhibits a subtle bluish tint, hinting at ongoing star formation. The overall morphology appears relatively smooth, lacking prominent spiral arm structures. There is some minor visual evidence of asymmetry within the disk, possibly indicative of minor gravitational interactions.
