The galaxy presents as a centrally concentrated, elliptical morphology. Its light profile appears relatively smooth, lacking significant spiral arm structures or prominent dust lanes. There's a slight elongation, deviating from a perfectly circular shape. The central region exhibits a bright, concentrated core, which is indicative of a possible supermassive black hole. The colour gradients suggest a redder hue in the central bulge, transitioning to slightly bluer tones in the outer regions, potentially indicating differences in stellar populations or star formation activity. There appears to be no major tidal disturbances or signs of ongoing mergers with other galaxies. Overall, this galaxy seems to be a relatively undisturbed, mature elliptical galaxy at a moderate redshift.
