The galaxy presents as a spiral structure with a notably elongated morphology, suggesting a moderate inclination relative to our line of sight. Spiral arms are clearly visible, extending from a central bulge region. The arms exhibit a patchy texture, indicative of active star formation regions. The central bulge appears relatively small and loosely defined, not exhibiting the characteristics of a dominant, classical bulge. Some asymmetry in the spiral arm structure is present, which could possibly indicate ongoing minor interaction or disturbance. The galaxy does not show any signs of major merger activity. The color profile seems to be slightly bluer in the disk, perhaps due to star formation. The galaxy is likely at a moderate redshift.
