The galaxy presents as a spiral galaxy, with a relatively high inclination angle, near edge-on. A distinct disk structure is observed. The primary color of the disk appears bluish, suggesting the presence of younger, hotter stars and ongoing star formation within the spiral arms. There is indication of significant star formation activity. A bulge component is visible, appearing more yellow and concentrated. This suggests an older stellar population with less active star formation. The galaxy shows some morphological disturbance. There may be minor interactions with a galaxy nearby. No major mergers are apparent from this image.
