The galaxy presents as a concentrated, yellowish-white central region. The morphology appears generally smooth, with a slight elongation. The galaxy exhibits a relatively high degree of central concentration, with light intensity decreasing gradually toward the outer edges. There is no apparent disk structure. Faint disturbances are present in the halo. The redshift of 0.134906 indicates a substantial distance, impacting the observed details. Overall, this galaxy appears to be in a late stage of evolution, or an elliptical galaxy with hints of recent interaction. Further spectroscopic analysis is warranted to fully characterize stellar populations, gas content, and dynamical state.
