The galaxy appears as a centrally concentrated object with a relatively smooth morphology. There is a dominant yellowish-white core suggesting a significant population of older stars. The overall shape is elliptical, tending toward an in-between or slightly rounded appearance. There is little evidence of spiral arm structure or a prominent disk; the galaxy is primarily spheroidal. No major merger events are apparent, nor significant tidal disturbances. The galaxy appears isolated. Color gradients suggest a possible evolution in stellar populations from core to halo, but it is difficult to discern any finer details. The apparent size is relatively small suggesting a moderate distance. Overall, it seems to be a fairly quiescent and well-established galaxy.
