The galaxy presents as a relatively smooth, elliptical or lenticular system. It possesses a centrally concentrated light profile, indicative of a large bulge. The overall color suggests a population of older stars. The galaxy appears relatively isolated, exhibiting no obvious signs of recent or ongoing major mergers or significant tidal interactions. The presence of color variation and asymmetry implies that the object may not be completely relaxed and may have undergone some recent interaction or accretion event. Star formation rates are likely suppressed in the galaxy and the morphology is consistent with a more evolved system.
