This galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. Its overall color suggests a population of older stars, with a generally reddish hue. The galaxy exhibits a high degree of radial symmetry, with isophotes appearing largely round, with perhaps a slight deviation. There are no prominent features like spiral arms or dust lanes visible. There is a hint of a faint halo surrounding the galaxy. The galaxy appears relatively undisturbed, showing no strong signs of major recent merger activity or tidal interactions, although the possibility of a minor interaction cannot be completely excluded. The star formation activity appears to be relatively low, consistent with the aged stellar population inferred from its color.
