The galaxy presents a generally smooth, elliptical morphology. Its core is highly luminous, with a concentration of light suggesting a significant stellar population and, potentially, an active galactic nucleus. The light becomes more diffuse towards the edges, with a slightly elongated form, not perfectly spherical. Faint color variations are observed within the galaxy, with a hint of bluer light at the edges and redder light at the center. The overall color suggests an older stellar population, and the lack of distinct spiral arms or strong dust lanes reinforces this, suggesting a relatively low star formation rate at present. A close inspection indicates the possibility of some minor tidal disturbances, possibly from a past interaction with a smaller galaxy, or the process of merging with one. This galaxy is of considerable mass and, assuming the red shift is accurate, is at a considerable distance.
