The galaxy presents a generally smooth morphology, appearing relatively undisturbed. It is elliptical in shape, with high degree of roundness. There is no apparent disk structure and no significant signs of recent or ongoing merger activity are observed, although a very minor perturbation cannot be completely ruled out. The color is generally consistent, with a slightly yellowish hue, indicating an older stellar population, with little on-going star formation. The galaxy is relatively bright, suggesting a large number of stars. The size is consistent with that of a moderate-sized galaxy.
