The galaxy presents as a spiral with a prominent disk structure. Spiral arms are clearly visible and well-defined, appearing somewhat tightly wound. The central bulge is moderate in size and exhibits a higher surface brightness compared to the disk. The galaxy shows a slight inclination relative to our line of sight. A faint stellar halo may be present, extending beyond the bright disk. There are no obvious signs of a major merger, though minor disturbances or interactions cannot be ruled out based solely on this image. The color indices suggest ongoing star formation, particularly within the spiral arms.
