The galaxy presents as an elongated, lenticular structure with a smooth, diffuse morphology. The central bulge exhibits a yellow-orange hue, suggesting an older stellar population. Moving outwards, the disk appears bluer, possibly indicating more recent star formation. No distinct spiral arms or bar features are discernible in the image. There appears to be little dust obscuration. The galaxy's smooth appearance suggests it is likely an early-type spiral or lenticular galaxy. The relatively high degree of roundness suggests a disk component with limited spiral structure. There are no obvious signs of recent major merger activity or significant tidal disturbances affecting its overall structure.
