The galaxy presents a discernible disk structure with prominent spiral arms. The arms appear relatively well-defined, exhibiting a winding pattern that transitions from medium to loose as they extend outwards from the galactic center. The galaxy has an apparent central bulge, although the exact size of the bulge is difficult to accurately determine, it seems to be a moderate size. Signs of star formation are evident, distributed throughout the spiral arms. Evidence of some level of interaction or disturbance is present, though it remains unclear if this is indicative of a minor or major interaction event. The overall color profile suggests a relatively active galaxy with ongoing star formation. The system is observed at a redshift, indicating a considerable distance. The apparent size is relatively compact.
