The galaxy presents as a spiral type, exhibiting well-defined spiral arms that wind tightly around a central bulge. The bulge appears relatively small compared to the overall disk size. A stellar bar structure seems to be present across the bulge. The spiral arms are not uniformly colored, but appear patchy with regions of blue interspersed with less prominent redder areas, suggesting ongoing star formation. The morphology of the arms suggest that a relatively high number of arms are present. No strong signs of tidal interactions are apparent in the image, but there could be some minor distortion of the spiral arms. The galaxy is viewed at a slight angle but appears mostly face-on.
