The galaxy presents as a somewhat elliptical or lenticular structure, exhibiting a prominent central bulge with decreasing luminosity extending outward. The core is bright and concentrated. Hints of a disk-like component are present, though features are not sharply defined. Patches of bluer light are visible in the outer regions, suggesting areas of star formation. Some faint irregularities are visible, indicating possible past interactions or disturbances. There does not appear to be significant ongoing major merger activity present. Overall, the galaxy shows a mixture of smooth, spheroidal components and fainter disk features.
