The galaxy presents as a moderately inclined, disc-shaped structure. The central region appears as a bright, concentrated bulge, indicating a significant stellar density. The disc component exhibits a smooth texture, suggesting a lack of prominent spiral arms. There is some evidence of a faint, diffuse halo extending beyond the main disc, though the boundaries are not sharply defined. The overall color is dominated by yellow-red hues, but there are also areas of blue-white hinting at more recent star formation regions in the disk. The outer edges of the galaxy exhibit lower surface brightness. The morphology suggests that the galaxy is an intermediate-type spiral.
