The galaxy presents a generally smooth and elliptical morphology. Its light is concentrated toward the center, exhibiting a bright, yellowish core. The radial distribution of light appears relatively uniform without distinct spiral arm structures or prominent dust lanes. The overall color suggests an older stellar population with low ongoing star formation activity. There is no obvious visual indication of any recent or ongoing merger events or tidal disturbances affecting the galaxy. The outer regions fade gradually into the background, indicating a well-defined but diffuse galactic halo.
