The galaxy presents as a somewhat amorphous, diffuse structure, exhibiting a yellowish hue that suggests an older stellar population. The central region appears slightly brighter, possibly indicating a concentration of stars or a galactic bulge. While there is some suggestion of faint spiral arms, the overall morphology is more akin to an elliptical or lenticular galaxy. There is some clumpy structure, but overall the galaxy is relatively smooth. There may be evidence of a small merger taking place, as indicated by some slight distortion of the shape. 
