The galaxy appears to be a luminous, elliptical-like system with a smooth, concentrated light profile. There is a dominant central bulge, which displays a yellow hue, likely indicative of an older stellar population. Fainter and bluer light surrounds the bulge, possibly indicating more recent star formation in the outer regions of the galaxy. The galaxy shows an apparently spherical shape. There is no obvious evidence of spiral arm structure. Faint tidal features are not apparent around the galaxy, suggesting it is not undergoing a major merger event, although minor disturbances could be present but are difficult to discern. 
