The galaxy appears to be a relatively smooth, elliptical galaxy with a bright, concentrated core. The light distribution suggests a high degree of central concentration, with a gradual decline in brightness towards the outer regions. There is a slight elongation, indicating it is not perfectly spherical. The color gradient shifts from a yellowish-white center to a bluer halo. No obvious spiral arms or dust lanes are discernible. There is little sign of active star formation, the light is mostly from an older stellar population.
