The galaxy presents as a single, dominant object with a largely spheroidal morphology. The light distribution appears smooth and concentrated towards the center, suggesting a high degree of central mass concentration. There is no readily discernible spiral structure or prominent disk.

The galaxy's color profile shifts from a yellow-white core to a faint reddish-brown halo, indicating an aging stellar population with a lack of recent or ongoing star formation. The absence of blue light suggests a dearth of young, hot stars within the galaxy.

There are no visible tidal tails, plumes, or obvious signs of interaction or merger events. The galaxy appears relatively undisturbed, exhibiting an elliptical or lenticular morphology.
