The galaxy presents as a disk galaxy, observed at a significant edge-on inclination. A prominent central bulge appears a yellow-orange hue. This suggests a higher concentration of older stellar populations in this region. Fainter bluish light along the visible edges of the disk indicates ongoing or recent star formation, albeit at a seemingly lower rate. The galaxy lacks a clear spiral arm structure, which is likely due to its edge-on orientation obscuring the arms. There are no visible signs of any major ongoing merger events or significant tidal disturbances. The morphology suggests a relatively undisturbed galactic structure.

