The galaxy presents as a centrally concentrated object with a generally smooth morphology, though some subtle features are discernible. The core region appears bright and yellowish-white, indicative of a population of older stars. Extending outward from this core is a fainter, bluer halo. The bluer color suggests the presence of some younger stars. The shape of the galaxy is somewhat elliptical, but there's a slight irregularity or possible faint disk-like structure hinting at some rotational support. There is no strong indication of recent major merger activity, but some minor disturbances are possible. Overall, the galaxy exhibits characteristics consistent with an intermediate type, possibly an early spiral or a lenticular galaxy transitioning from a more active star-forming state to a more quiescent state.
