The galaxy presents a clear spiral structure, although the arms appear tightly wound. The central bulge is prominent and moderately sized, contributing significantly to the overall luminosity. The disk is inclined relative to our line of sight, appearing somewhat elliptical. Color gradients suggest ongoing star formation within the spiral arms, exhibiting a bluer hue compared to the more yellowish central bulge, where older stellar populations likely dominate. There is no apparent sign of a major merger or significant disturbance in the galaxy's overall structure.
