The galaxy presents as a spiral galaxy with a substantial disk component. The spiral arms are tightly wound around a moderately sized bulge, appearing tightly packed, and are relatively distinct and well-defined. There is evidence of two prominent spiral arms. The central bulge exhibits a yellowish-orange hue, potentially indicating an older stellar population, whereas the disk shows a bluer color, suggesting ongoing star formation. The galaxy appears relatively undisturbed, displaying no obvious signs of a major merger event. The galaxy is not perfectly edge on, but shows a slight angle.