The galaxy presents as a yellowish-white elliptical shape with a smooth morphology. A slight extension is observed along what appears to be its major axis. The light distribution suggests a high degree of central concentration, though it is largely diffuse. A distinct nucleus can be observed in the very center, and there may be a second nucleus in the surrounding halo. There are no apparent spiral arm structures or dust lanes visible in this observation. Overall, the galaxy appears relatively undisturbed and does not show strong indications of recent major mergers or tidal interactions. The colors suggest an older stellar population.
