The galaxy presents as a spiral type, characterized by a prominent central bulge and well-defined spiral arms. The bulge exhibits a smooth, yellowish hue, suggesting an older stellar population. The spiral arms are tightly wound around the bulge, displaying a bluish tint indicative of ongoing star formation. Patchy regions of star formation are apparent along the arms. The dust lanes appear to be distinct, and the disk appears relatively undisturbed. The galaxy's orientation is close to face-on, with a moderate bulge size.
