The galaxy presents a largely smooth, elliptical morphology with a high degree of central concentration. It appears nearly spherical, with only slight deviations from perfect roundness. The color profile suggests an older stellar population, with a dominant yellowish-orange hue in the central regions. This likely indicates a lack of significant ongoing star formation. There are no readily apparent spiral arms, bars, or other disk-like features. No significant signs of recent or ongoing merger activity are detected. The overall appearance suggests a quiescent, evolved galaxy.
