The galaxy presents a yellowish-white hue, suggesting a significant population of older stars. Its morphology appears largely smooth and elliptical. The galaxy has a high concentration of light in its core region, indicating a possible supermassive black hole actively accreting material. There are two distinct centers of light concentration in the galaxy, with one being slightly more diffuse than the other. These may be two galaxies in the process of merging. Overall, the object shows a relatively smooth and undisturbed structure, although the two distinct light concentrations make the structure a little unusual.
