The galaxy presents as a spiral type, exhibiting a notable disk structure. Multiple spiral arms emanate from the central bulge, displaying a tightly wound morphology. The color distribution suggests ongoing star formation within the arms, indicated by the presence of bluer regions. A prominent central bulge is observed. No significant evidence of a major merger is apparent, although some minor disturbances or irregularities in the arm structure are observed. The orientation of the disk is close to face-on relative to our line of sight, allowing for detailed examination of the spiral arm structure. The overall color profile indicates a relatively high luminosity object with a considerable stellar mass.
