The galaxy presents a generally smooth morphology. Its light profile appears centrally concentrated, with a high degree of radial symmetry. The ellipticity is moderate, suggesting a classification somewhere between an elliptical and a lenticular galaxy. There is a clear color gradient, with the central region exhibiting a more yellow/orange hue. Moving outward from the center the galaxy becomes bluer, suggesting the possibility of a younger stellar population at the outer edges. There are very faint hints of subtle disturbances, however overall, the object does not show any obvious signs of recent major merger activity.
