The galaxy exhibits a somewhat flattened, elliptical morphology with evidence of a disk structure. The central region displays a higher surface brightness, suggestive of a central bulge, though it does not appear overwhelmingly dominant. Faint spiral arm structures are discernible, though not sharply defined, indicating a spiral galaxy classification. The galaxy appears to be undergoing star formation as evidenced by the bluish color in the arms. The overall color suggests a redshifted system, with a blend of both older stellar populations and ongoing, perhaps moderate, star formation. There are no obvious signs of a recent major merger. There is minor structural irregularity, suggesting some gravitational disturbance.
