The galaxy presents a disk-like morphology, inclined relative to our line of sight. A central bulge region is evident with a yellowish hue, suggesting an older stellar population. Fainter spiral arms extend outward from the bulge. The arms appear bifurcated and somewhat tightly wound. The overall color suggests moderate star formation activity is present. No obvious signs of major mergers are visible, but some minor irregularities in the disk structure might indicate past or ongoing gravitational interactions. A faint bar-like structure appears to be present in the center of the galaxy.
