The galaxy presents as an elliptical or lenticular structure, appearing largely smooth and featureless. The light is concentrated towards the core, with a gradual decrease in intensity outwards. The central region exhibits a yellowish hue, possibly indicating an older stellar population. There is a faint, bluer outer halo. No spiral arms or distinct dust lanes are discernible. The galaxy appears relatively isolated with no signs of tidal disturbances or interaction with other galaxies. The overall morphology suggests a system where star formation is not currently a dominant process.