The galaxy appears as a relatively smooth, centralized object with a slightly oblate spheroidal morphology. Its color is generally muted, leaning towards the redder end of the spectrum. There is minimal evidence of spiral arm structures or significant dust lanes. The galaxy appears centrally concentrated, with a gentle decrease in luminosity outwards from the core, this indicates there is no strong sign of it being disturbed by any recent merging activity. The absence of strong blue regions suggests a generally low rate of on-going star formation. The redshift indicates that we are observing this galaxy at a considerable cosmological distance, so many morphological features are hard to discern.
