The galaxy presents as a centrally concentrated, largely featureless spheroid, consistent with an elliptical morphology. The color gradient transitions from a yellowish-white core to a reddish outer halo. There is no apparent spiral structure or dust lane visible. The galaxy appears to be fairly isolated, with no obvious signs of tidal distortion or close companions. The high degree of central concentration suggests a significant bulge component. The smooth appearance and redder color indicate an older stellar population and reduced ongoing star formation. The shape of the galaxy approximates a sphere, with minor deviations from perfect circularity.
