The galaxy presents as an elliptical morphology. It exhibits a centrally concentrated bulge that appears largely smooth, with a gradual decline in luminosity extending outwards. The core of the galaxy has a yellowish hue, possibly indicating an older stellar population. Fainter bluish regions are observed around the core, indicating younger star formation. The galaxy shows no obvious signs of spiral arm structures. It appears to have undergone relatively undisturbed evolution. Overall, the galaxy exhibits characteristics consistent with an elliptical galaxy containing a population of both old and young stars.
