The galaxy presents as a smooth, elliptical structure with no discernible spiral arms or bar features. Its light is dominated by a yellowish-white hue concentrated towards the center, suggesting an older stellar population and relatively low star formation activity. The galaxy exhibits a slight elongation, appearing more oblate than perfectly spherical. There is minimal evidence of dust lanes or prominent HII regions. The overall appearance suggests a relaxed, dynamically stable system with no obvious signs of recent major mergers or significant tidal disturbances, though some minor asymmetry is present. The galaxy's color profile is consistent with that of a red sequence galaxy, indicating a high mass and predominantly passive stellar evolution.
