The galaxy presents as a relatively smooth, elliptical-like structure. The central region is a bright yellowish-white, which may indicate an older stellar population dominating the core, or possibly a highly redshifted population of stars that is naturally redder than the light from similar stars closer to us. The galaxy does not show prominent spiral arms or a well-defined disk. There are faint extensions around the central region. Overall, the galaxy appears to be a relatively undisturbed system, with no apparent major merging events.
