The galaxy presents as a spiral type, exhibiting a relatively high degree of rotational symmetry. Spiral arms are clearly visible, demonstrating a tightly wound morphology. The central bulge appears moderate in size relative to the overall galactic disk. The light distribution suggests a relatively smooth disk component, with no obvious major disturbances or signs of ongoing major merger activity. Star formation appears to be ongoing, particularly within the spiral arms, as indicated by the presence of bluer regions. The galaxy is slightly elongated, with an apparent axis ratio close to 1. The spiral arms are traced by areas of enhanced blue luminosity, indicative of younger stellar populations. Overall, it appears to be a disk galaxy of substantial mass with moderate star formation activity and tightly wound spiral structure.
