The galaxy presents as a relatively smooth, elliptical structure. Its core exhibits a high degree of central concentration, with a bright, yellowish-white luminosity suggesting an older stellar population dominating this region. Moving outwards from the core, the light gradually diminishes. There is a very faint disk present, and the overall distribution of light appears undisturbed, without evidence of significant tidal features or ongoing mergers. The morphology appears largely undisturbed. The redshift indicates the galaxy is at a considerable distance.
