The galaxy presents a distinct spiral structure. The spiral arms are tightly wound around a prominent central bulge, indicating a possible Sa or Sb classification. The bulge appears relatively large, contributing significantly to the overall luminosity of the galaxy. There's a subtle suggestion of a bar structure bisecting the bulge, although it's not strongly defined. The arms exhibit a flocculent, patchy appearance, suggesting ongoing star formation activity within the disk. The color distribution indicates a mix of stellar populations, with a yellowish-red core likely composed of older, redder stars and bluer regions in the spiral arms indicative of younger, hotter stars. There are some indications of minor disturbances in the outer regions of the disk which could indicate a past merger or interaction.
