The galaxy presents as a moderately bright, elliptical system with a noticeable central bulge. The light distribution suggests a relatively smooth morphology with a high degree of central concentration. The galaxy exhibits a color gradient, with a yellowish-white core gradually transitioning to a fainter, redder halo. There is some suggestion of a very subtle disk component, though the light is dominated by the bulge. The isophotes appear largely undisturbed. The system displays no obvious signs of major mergers or significant tidal features. The galaxy is likely at a considerable distance, based on its redshift, and the apparent size suggests a reasonably sized galaxy.
