The galaxy presents as a relatively smooth, elliptical-like structure with a central bulge that appears to be a more concentrated region of luminosity. There is no clear spiral arm structure visible. The overall color of the galaxy exhibits a reddish-orange hue, possibly indicating an older stellar population and a relatively low rate of ongoing star formation. The galaxy displays a high degree of rotational symmetry. There is some slight irregularity visible, although it is unclear if this is due to a minor interaction or disturbances, or simply image noise.
