The galaxy presents a relatively smooth, elliptical morphology with a concentrated central bulge that appears bright and yellowish-white in color. The overall shape is roughly circular, but with a slight elongation along one axis. There are no discernible spiral arms or prominent dust lanes visible. A faint, bluish halo surrounds the central region, suggesting the presence of some younger stellar populations, although the dominant color indices indicate a more mature stellar population overall. There are no obvious signs of significant recent merger activity or major disturbances in the galaxy's structure, but there may be some minor asymmetry or subtle features suggesting a possible past interaction or ongoing internal dynamics.
