The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical with a high degree of roundness. There is a dominant central bulge that radiates outwards into a more diffuse halo. There is no discernible spiral structure or bar. The galaxy exhibits a color gradient, transitioning from a yellowish hue at its core to a slightly redder tinge in the outer regions, possibly indicating a difference in stellar population ages or dust distribution. No prominent dust lanes or tidal features are readily apparent. The overall structure suggests a lack of recent major merger events. The galaxy's form appears generally undisturbed, indicative of a relatively quiescent evolutionary state.
