The galaxy presents as a primarily smooth, elliptical-like structure. The light is centrally concentrated with a gradual decrease in intensity moving outwards. The overall color appears to be in the redder part of the spectrum. There is some evidence of a subtle flattening, but it is largely spheroidal in appearance. There is no strong evidence of spiral arms, bars, or significant dust lanes within the galaxy. The surrounding region appears relatively undisturbed, with no obvious tidal features or nearby companions suggesting a recent major merger. The light distribution suggests an evolved stellar population, with minimal ongoing star formation visible in this imagery.
