The galaxy presents as a relatively smooth, elliptical-like structure. Its light profile appears centrally concentrated, with a bright, yellowish core that gradually diffuses outwards. The isophotes are generally rounded, exhibiting only a slight elongation. There is no discernible evidence of spiral arms, bars, or significant dust lanes. The color suggests a predominantly older stellar population, consistent with a quiescent or passively evolving galaxy. The overall structure indicates that it does not appear to be undergoing any major merging events or significant tidal interactions.
