The galaxy presents as a concentrated, relatively smooth object. It exhibits a generally elliptical morphology, appearing mostly round with slight elongation. There is a noticeable color gradient, with the core appearing more yellow. The outer regions fade into redder hues, suggesting an aging stellar population with little active star formation. No spiral arm structures or dust lanes are clearly visible. The overall appearance suggests this is a large, massive system at a significant cosmological distance, likely with a relatively low star formation rate. There is no evidence of any major ongoing mergers or significant tidal disturbances.
