The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. There is no apparent disk structure or spiral arms. The galaxy appears largely featureless, showing no evidence of significant dust lanes, tidal tails, or ongoing major merger activity. A slight elongation is visible, deviating from a perfectly circular shape. Color gradients indicate a central region that is notably redder and brighter compared to its fainter, bluer outer regions. This color difference suggests an older stellar population dominates the galaxy's core, while younger stars may exist in the surrounding areas. Overall, the galaxy exhibits characteristics consistent with a mature, relatively quiescent system.
