The galaxy presents a smooth, elliptical morphology with a concentrated central bulge. The light distribution is relatively uniform, exhibiting a gradual decrease in intensity from the core to the outer regions. There is no discernible spiral arm structure or significant dust lane obscuration visible in this image. The color appears to be dominated by older stellar populations, indicated by the yellowish hue. The overall appearance suggests a mature galaxy that has largely completed its star formation phase. A slight asymmetry may be present but is not highly obvious. There is no evidence of ongoing major mergers or significant tidal disturbances. 
