The galaxy presents a largely smooth, elliptical morphology with minimal discernible substructure. The light profile exhibits a concentrated core, indicative of a high degree of central mass concentration. A faint disk-like structure, slightly offset from the core, is oriented roughly vertically. The color gradient suggests older stellar populations are dominant, with a central concentration of older, redder stars. The galaxy displays a moderate redshift, suggestive of significant distance. There is no indication of ongoing major merger activity, though a slight asymmetry in the outer halo could indicate a minor interaction or disturbance. Overall, the galaxy appears to be a relatively evolved system, transitioning towards a quiescent state with suppressed star formation.
