The galaxy presents a largely smooth and concentrated appearance, with a high degree of central luminosity that diminishes gradually towards the outer edges. The overall shape is somewhat elliptical, appearing elongated rather than perfectly spherical. The color profile indicates a relatively older stellar population, with a bias toward redder hues though bluer wavelengths can still be perceived. No prominent spiral arms or distinct features are visible. There's a subtle suggestion of minor asymmetry or disturbance in the outer regions, potentially indicative of past interactions or minor merging events. The galaxy shows signs of low star formation activity.
