The galaxy presents as an elliptical morphology, appearing generally smooth and rounded. A concentrated central bulge exhibits a yellowish-white hue, suggestive of an older stellar population. The outer regions of the galaxy fade gradually, displaying a bluer color, which may indicate some ongoing, although potentially low, levels of star formation activity. There are no apparent spiral arm structures or significant dust lanes visible in the image. The overall shape is relatively symmetric, showing no obvious signs of major disturbances or ongoing mergers.
