The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, with a high degree of roundness. The galaxy's light profile appears to gradually decrease outwards from the center, with no obvious spiral arm structure or distinct features. The central bulge is prominent and appears to be composed of an older stellar population, indicated by its yellow-white color. A faint halo or extended envelope of stars surrounds the main body of the galaxy. There are no signs of a major ongoing merger, although some minor disturbances may be present in the outer regions.
