The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a bright central bulge, with luminosity decreasing gradually towards the outer regions. The light distribution appears largely symmetrical. There is a slight yellow-orange hue to the galaxy overall, with a higher concentration of yellow light emanating from the central region. There is no apparent spiral structure or prominent dust lanes that are visible at this resolution. The overall shape is close to round, with no obvious elongation. There is no evidence of strong tidal distortions or merger activity, although the possibility of a minor disturbance cannot be ruled out. Star formation rate appears to be low.
