The galaxy presents a distinct spiral structure, although the spiral arms are not sharply defined. They appear somewhat tightly wound around a moderate-sized central bulge. The bulge exhibits a yellowish-white hue, suggesting an older stellar population. The spiral arms display a bluer color, likely indicating ongoing star formation. There's a hint of a bar-like structure traversing the central region, although it's not very prominent. The galaxy shows no obvious signs of a major merger, though there might be some minor irregularities hinting at a possible disturbance. Overall, the galaxy appears as a relatively normal spiral galaxy with moderate star formation activity.
