The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal in shape. A concentration of light towards the center indicates a prominent galactic bulge. There is a color gradient visible, transitioning from a yellowish-white core to a bluer halo. The yellowish core suggests an older stellar population, while the bluer outer regions may indicate the presence of younger, hotter stars or ongoing star formation, albeit at a low rate. The overall structure shows no signs of significant tidal disturbance or ongoing major merger activity, although some minor distortions may be present. The galaxy's apparent roundness points away from a highly inclined disk-like structure.
