The galaxy appears as a centrally concentrated object with a fairly smooth, elliptical morphology. The core exhibits a yellowish-white hue, suggesting a concentration of older stellar populations. Fainter, bluish-tinged outer regions extend from the central bulge, indicative of some ongoing, though perhaps limited, star formation. There is no clear spiral structure or distinct disk readily apparent. The overall light distribution is relatively smooth with some subtle asymmetries, but these do not strongly suggest a major ongoing merger event. There is no apparent tidal debris or extended features to indicate any recent interaction with another galaxy. The galaxy's apparent roundness suggests it may be an E0-E2 elliptical, viewed close to face-on.
