The galaxy presents as a largely smooth, elliptical-like structure. There is a concentrated central bulge of significantly higher luminosity relative to the surrounding galactic halo. The galaxy appears to be quite evolved, as implied by its lack of resolved star-forming regions and predominantly smooth morphology. There appears to be little if any disk-like component, and no evidence of spiral arms or other significant structural features, suggesting that this galaxy is undisturbed. It appears to be quite massive. The overall color of the galaxy is relatively red, likely indicative of an older stellar population and a low star formation rate. There is no visual evidence of any ongoing merger activity or significant tidal disturbances.
