The galaxy presents as a centrally concentrated, generally smooth structure. Its overall morphology appears to be elliptical or lenticular, with a high degree of circularity. There is a subtle color gradient; the core of the galaxy displays a slightly redder hue, possibly indicating an older stellar population. The outer regions are less distinct, suggesting a lower surface brightness. There is no prominent disk structure or spiral arm features. The galaxy does not exhibit any apparent signs of tidal disturbances or ongoing merger activity; it appears isolated and undisturbed. The relative smoothness suggests that its star formation rate is generally low. 
