The galaxy appears to be a relatively smooth, elliptical galaxy. Its core has a diffuse light distribution which smoothly fades toward the edges. The morphology suggests a spheroidal shape, with no prominent spiral arms or significant disk features visible. Its generally smooth appearance is indicative of an older stellar population.

There are subtle color variations across the galaxy, though they may be subtle image processing effects. These color variations may also indicate differing stellar populations or dust content within the galaxy. There is no visible sign of any ongoing major merging activity or significant tidal disturbances. The light profile has a high degree of radial symmetry.
