The galaxy presents as a well-defined elliptical system with an estimated redshift suggesting it is relatively distant. The morphology indicates a smooth, featureless structure, with a high degree of central concentration. The galaxy displays a pronounced bulge component with a relatively high Sersic index. Color gradients suggest a population of older stars, with the central region exhibiting a yellower hue. The overall shape is moderately elliptical, exhibiting a moderate flattening. There is no evidence of spiral arms, dust lanes, or other distinct features typically associated with disk galaxies or active galactic nuclei.
