The galaxy presents as an elliptical or lenticular structure, characterized by a high degree of central concentration. The light distribution is relatively smooth. There is a bright, prominent central bulge with a yellowish hue. The outer regions display a less intense, greenish color. There is little to no visible dust or spiral arm structure. The galaxy appears generally round in shape with no obvious signs of tidal disturbances or interactions. The overall morphology suggests a relatively evolved system with a dominant stellar population. 
