The galaxy presents a primarily smooth morphology, with a somewhat elliptical shape. The light distribution is centrally concentrated, showing a gradual decrease in intensity moving outward from the core. The galaxy appears largely featureless, lacking prominent spiral arms or strong dust lanes. The core exhibits a yellowish-white hue, suggestive of an older stellar population. The outer regions display a slightly redder tint, likely due to the presence of cooler, older stars. No significant signs of ongoing major mergers or tidal disturbances are apparent. Based on its redshift, this galaxy is at a considerable distance. The inferred absolute magnitudes place it among relatively luminous galaxies. Overall, the galaxy appears to be a relatively massive early-type galaxy with a low star formation rate.
