This galaxy presents a distinct spiral morphology, exhibiting prominent arms that contribute significantly to its overall structure. The arms appear somewhat tightly wound around a central bulge, indicative of a Sb or Sc classification. The bulge region displays a moderate size relative to the galaxy's disk. While a bar structure is not definitively observed, a subtle elongation could suggest a weak bar presence. Star formation activity appears evident, particularly within the spiral arms, as indicated by the observed blue color. A slight asymmetry or disturbance suggests the possibility of a minor interaction or merger event in its past. Overall the galaxy appears as a well-defined spiral with a classical structure, and a moderate redshift.
