The galaxy presents as an elliptical morphology, exhibiting a high degree of smoothness and a centrally concentrated light profile. The core region displays a bright, yellowish hue, likely indicating an older stellar population. There is a gradual decrease in luminosity from the center outwards. No prominent spiral arms or distinct disk-like structures are visible. The overall shape is largely rounded and undisturbed, with minimal evidence of tidal features or ongoing merger activity. The color suggests relatively low levels of on-going star formation.
