The galaxy appears to be a relatively smooth, elliptical galaxy at a moderate redshift. The morphology indicates a well-defined central bulge, lacking any prominent spiral arm structure or significant dust lanes. The light distribution suggests a high degree of central concentration, with a gradual decrease in luminosity towards the outer regions. It is generally round in shape. There is no visible evidence of any current major mergers or tidal disturbances. The galaxy appears to be a relatively isolated system. It displays a blue tinge near the center suggesting the presence of some younger stars, but overall, the light is redder than pure blue, indicating an older stellar population.
