The galaxy presents as a relatively smooth, elliptical-like structure. Its light profile increases towards the center, with the core being the brightest region. There is a slight elongation that is close to round, and appears to have no significant disturbances or signs of a major merger event. The outer regions of the galaxy display a gradual fading in luminosity. Color gradients suggest the possibility of some ongoing star formation activity, or at least the presence of a younger stellar population compared to a completely quiescent system.
