The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a largely elliptical morphology, appearing quite rounded in shape. A slight elongation is possibly detected in the galaxy's overall structure. There is a subtle color gradient visible, transitioning from a more blueish hue towards the center, likely indicating a region of higher star formation, to redder tones in the outer regions. This suggests an aging stellar population residing further from the core. Possible minor disturbances are exhibited, as there is a slight distortion to the smooth shape of the galaxy.
