The galaxy presents a primarily smooth morphology, exhibiting a centrally concentrated bulge. The overall shape is largely spheroidal, although there's a slight elongation visible, deviating somewhat from a perfectly circular profile. The galaxy displays a color gradient, appearing more yellow at the core, suggesting a population of older stars. There is an absence of clearly defined spiral arms or other distinct features. Based on the observed color and morphology, this galaxy likely has a low star formation rate and a considerable stellar mass. Minimal evidence of recent or ongoing mergers can be observed, and disturbance from a major external event is unlikely.
