The galaxy presents as a concentrated, ellipsoidal structure, exhibiting a high degree of central luminosity. The morphology appears largely smooth, lacking prominent spiral arms or significant dust lanes. The light distribution suggests a relatively homogenous stellar population. The galaxy appears relatively isolated, without obvious signs of tidal interactions or ongoing mergers. Color gradients indicate a potential concentration of older stellar populations towards the galactic core. The absence of distinct features points to a classification as an elliptical or lenticular galaxy. There may be a slight asymmetry in the outer isophotes, though this could be a result of image artifacts. Overall, the galaxy seems to be a relatively evolved system, exhibiting little evidence of recent star formation.
