The galaxy presents a largely smooth, elliptical morphology. There is a high degree of central concentration, with the light appearing brightest at the core and gradually diminishing outwards. The galaxy exhibits a golden hue, suggesting a stellar population dominated by older, redder stars. No distinct spiral arms or disk-like features are discernible. The overall shape appears nearly circular, with a slight elongation. There is no obvious evidence of recent or ongoing major mergers or significant tidal disturbances.
