The galaxy appears to be a relatively smooth, elliptical-like structure. Its overall color suggests a mature stellar population. There appears to be little evidence of recent major merger activity or significant tidal disturbances, though there may be a slight asymmetry to its outer regions. The galaxy's roundness suggests that any rotational support is limited, and its luminosity indicates a massive galaxy. Star formation appears to be suppressed within the galaxy, with a low specific star formation rate.
