The galaxy appears to be an elliptical galaxy with a smooth, spheroidal morphology. The core exhibits a pronounced central bulge, characterized by a bright, concentrated luminosity profile, that quickly dissipates in intensity. A gradient in color from the core to the halo shows an age difference in the stellar populations. The core appears more orange, while the halo surrounding it is more greenish. The halo has a much fainter luminosity than the core. There is no visible indication of spiral arm structure or significant dust lanes. There seems to be no ongoing major merging events. The roundness of the galaxy is in between being perfectly round and oblong. There are no visible tidal features or disruptions indicating any recent interactions. The galaxy is estimated to be quite massive, based on its luminosity and size. The star formation rate is relatively low.
