The galaxy appears to be a relatively smooth, elliptical-like system. Its light profile is concentrated towards the center, with a bright, yellowish core indicative of an older stellar population. There is a gradual decrease in luminosity moving outwards from the core. The overall shape is somewhat elongated, though the light is distributed fairly evenly on either side of the major axis. Subtle hints of a disk-like structure may be present, but these features are not prominently defined. No significant signs of ongoing major mergers or tidal disturbances are readily apparent in the image.
