The galaxy presents as an elliptical or spheroidal structure with a high degree of central concentration. The core exhibits a yellowish-white hue, suggesting an older stellar population. The outer regions display a subtle greenish tint, potentially indicating a younger stellar population or emission from ionized gas. The overall smoothness of the galaxy indicates it is unlikely undergoing any major merger events. There is no evident spiral arm structure, or distinct disk visible. The galaxy appears to be relatively isolated and does not show signs of significant tidal disturbances.
