The galaxy presents as a relatively smooth, elliptical-like structure with a high degree of central concentration. The core exhibits a yellowish hue, indicative of an older stellar population. Moving outward from the core, a faint bluish halo is observed, potentially suggesting the presence of a younger stellar population or ongoing star formation at the galaxy's periphery, though the smoothness could suggest the blue light is simply the color of older, dimmer stars that are still present. The object's shape departs slightly from a perfect circle, hinting at an ellipsoidal morphology. There are no apparent signs of major disturbances or significant tidal features, although a subtle irregularity might suggest minor gravitational interactions. Overall, the galaxy appears as a relatively undisturbed, moderately massive system with evidence of both old and possibly recent stellar activity.
