The galaxy presents as a spiral galaxy viewed at a moderate angle, not quite edge-on. The central bulge appears relatively prominent, exhibiting a yellowish-white hue, suggesting an older stellar population. Fainter spiral arms extend from the central bulge, winding tightly around the center. The arm structure displays patchy regions of blue, indicating areas of recent star formation. A bar-like structure is present within the central region, though not sharply defined. There may be some minor disturbance or asymmetry in the outer regions of the disk, potentially due to tidal interactions, although no clear evidence of a major merger is immediately apparent. The overall appearance suggests a galaxy that is actively forming stars within its spiral arms.
