The galaxy presents as a spiral system, observed at a moderate inclination. A prominent central bulge dominates the galaxy's morphology, exhibiting a smooth, concentrated light profile that transitions into a less structured disk. The disk shows evidence of spiral arm structures, but they appear somewhat flocculent and not tightly wound. The arms exhibit a bluer hue compared to the bulge, indicative of ongoing star formation. Dust lanes appear to be present within the disk, obscuring portions of the spiral arms. The overall structure appears relatively undisturbed, showing no strong signs of major merging events or tidal distortions.
