The galaxy presents as a centrally concentrated, elliptical system at a redshift of approximately 0.22. Its overall morphology appears smooth with little visible substructure, suggesting a lack of significant recent merger activity or strong tidal interactions. The isophotes exhibit a generally rounded shape, deviating minimally from circularity, further indicating a relaxed dynamical state. Color gradients reveal a subtle bluing towards the outer regions, indicative of a change in stellar populations. The core of the galaxy is dominated by redder light, which suggests an older, more metal-rich stellar population. Star formation activity is low, indicating that it's likely a more evolved system.
