The galaxy presents as a relatively smooth, elliptical morphology with a moderately elongated shape. It exhibits a concentrated central bulge which appears to be composed of older stellar populations, suggested by its yellowish-orange hue. There is faint bluer light in the outer regions of the galaxy. There is no significant evidence of spiral arm structure or prominent dust lanes. A slight asymmetry is present, suggesting possible minor gravitational interactions, but no large scale disturbances are apparent. The overall color index suggests a passively evolving system with a low rate of ongoing star formation.
