The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The primary color is a yellowish-white, which suggests a population of older stars dominating the light output. The galaxy appears to be moderately distant, and shows no signs of distinct spiral arms or strong dust lanes. There's a very slight flattening which suggest it is not perfectly round. The smooth profile indicates that it has likely undergone significant dynamical relaxation over time, which also would explain its older stellar populations.
