The galaxy presents as a largely featureless, smooth object, exhibiting a high degree of central concentration. Its overall morphology appears elliptical, with an approximate roundness. There is little evidence of spiral arms or significant disk-like structures. The galaxy displays a distinct color gradient, transitioning from a yellowish-white core to redder outer regions. This color variation suggests a stellar population gradient, with potentially older, redder stars dominating the outer halo, and a younger population concentrated in the core. There are no indications of ongoing major mergers or significant tidal disturbances in this image. Faint asymmetries are observed but do not appear to be disruptive.
