The galaxy presents as a relatively smooth and centrally concentrated object. Its overall shape is elliptical, appearing nearly circular. The light distribution exhibits a radial gradient, brightest at the center and gradually decreasing towards the outer regions. The core appears bright yellow, likely indicating an older stellar population. There are subtle hints of some disturbances in the galaxy. There appears to be some blue light towards the edge of the galaxy, which could indicate a population of younger stars, with an ongoing, albeit low, rate of star formation. Overall, the galaxy gives the appearance of a massive and relatively evolved system.
