The galaxy presents a generally smooth morphology, with a high degree of roundness.  Color gradients suggest an evolved stellar population. The lack of discernible spiral arms or prominent features points to a structure that is likely an elliptical or lenticular galaxy. There is a possible faint, diffuse halo surrounding a brighter central bulge region. No signs of significant tidal disturbances or ongoing merger activity are apparent. The galaxy exhibits a redder color profile which is consistent with a galaxy at a redshift of approximately 0.14.
