This galaxy presents as a relatively compact and smooth elliptical or lenticular galaxy. It exhibits a high degree of central concentration with a bright, slightly elongated core. There is a subtle color gradient, the central region appears slightly bluer than the outer halo. Overall, the galaxy exhibits a smooth, diffuse light profile, suggesting an older stellar population with little active star formation. There is no obvious disk-like structure or spiral arms. Subtle distortions in the outer halo indicate there may have been minor gravitational interactions with another galaxy in the past.
