The galaxy presents as a largely featureless, smooth object. Its overall shape is elliptical, displaying a high degree of circularity with an almost perfect roundness. There is a concentrated central bulge that appears bright and luminous, likely indicative of a high density of stars. Moving outward from the core, the intensity of the light gradually diminishes into a faint, extended halo. No prominent spiral arms or dust lanes are discernible, suggesting a lack of significant ongoing star formation. The object seems to be relatively undisturbed, with no obvious signs of recent mergers or tidal interactions. The galaxy's color suggests an older stellar population, dominated by redder, more evolved stars, but with a hint of bluer stars in the core.
