The galaxy presents a generally smooth, elliptical morphology. Its light profile exhibits a high degree of radial symmetry and concentration. The central region is significantly brighter than the surrounding areas, indicating a substantial concentration of stars or potentially an active galactic nucleus (AGN). There is no discernible spiral arm structure, nor any obvious dust lanes.

The galaxy’s color is yellowish-orange, suggesting a population of older, redder stars. The relative lack of blue light indicates a low rate of ongoing star formation. It shows little to no signs of recent major mergers or tidal disturbances, exhibiting only a marginal asymmetry. The overall appearance is consistent with that of a massive, quiescent elliptical galaxy.
