The galaxy presents as a relatively smooth, elliptical-like structure. It has a dominant central bulge that appears yellowish-white, suggesting a population of older stars. There is a fainter, bluer halo that surrounds the bulge; the bluer hue could indicate regions of ongoing or recent star formation. There seems to be a disk-like structure, which may be rotating.

Some features that might be indicative of a minor disturbance are seen, perhaps a minor tidal interaction. There appear to be no strong tidal tails or other significant signs of a major merger event. Its overall appearance is not perfectly symmetrical, displaying a slight elongation. The light is concentrated in the center, fading outward toward the edges.
