The galaxy presents as a fairly smooth, elliptical or lenticular system. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. The color appears to be yellowish-white, indicating a population of older stars with a relatively low rate of ongoing star formation. There is a subtle hint of a disk-like structure, though no distinct spiral arms are visible. The overall shape is somewhat rounded but not perfectly spherical, appearing slightly flattened. No major disturbances or signs of an ongoing major merger event are evident, though there is a very slight asymmetry.
