The galaxy exhibits a spiral morphology, though the spiral arms are not sharply defined. The central bulge is prominent and displays a yellowish hue, suggesting an older stellar population. The disk component shows a bluer coloration compared to the bulge, indicative of ongoing star formation. There is some indication of a bar-like structure extending through the center of the galaxy, although it appears somewhat weak. The overall structure appears relatively undisturbed, with no obvious signs of major mergers or significant tidal distortions. A moderate amount of dust appears to be obscuring some of the light from the disk, making the spiral structure somewhat less distinct.
