This galaxy presents as a spiral galaxy, observed at a non-edge on angle. Evident are spiral arms that appear somewhat patchy, possibly indicating ongoing or recent star formation within these arms. A central bulge is visible, though it appears relatively small compared to the overall disc size. The galaxy exhibits a moderate degree of internal structure, not appearing entirely smooth. There's a suggestion of a bar-like feature spanning across the bulge. The color gradients imply variations in stellar populations or dust content throughout the galaxy, with the core region appearing more yellow/orange. The overall morphology does not suggest any major ongoing merger events.
