The galaxy presents as a somewhat smooth, elongated structure, with an overall cigar-shaped morphology. It exhibits a central concentration of light with a yellowish hue, potentially indicating an older stellar population. The outer regions show a gradual decrease in luminosity and appear slightly bluer, possibly indicative of more recent star formation. There may be some slight asymmetry in the outer regions, but no clear signs of major disturbances or ongoing mergers are readily apparent. Based on its form, this is likely an elliptical or lenticular galaxy. 
