The galaxy appears to be a spiral galaxy seen at a significant tilt relative to our line of sight, presenting an elongated, nearly edge-on profile. The light distribution suggests a central bulge, though it is not sharply defined. A disk component is evident, exhibiting a smooth texture with hints of spiral arm structure. The color gradient across the galaxy shows variations, possibly indicating differing stellar populations or dust lane presence. There may be ongoing, but not very intense, star formation activity. Based on the undisturbed morphology, no major recent merger events seem apparent, though minor interactions cannot be ruled out.
