The galaxy presents as a centrally concentrated, moderately luminous object with an overall elliptical morphology. Its color index suggests a redder, more evolved stellar population, consistent with a relatively low ongoing star formation rate. The light distribution appears largely smooth, with a high degree of central concentration and minimal evidence of spiral arm structure or significant dust lanes. The shape is closer to round, with very little elongation. There is a minimal indication of any tidal features or other morphological disturbances, suggesting it is not currently undergoing a major merger event, although there may be minor interactions occurring. Overall, the galaxy appears to be a relatively massive, quiescent system at a redshift indicative of a considerable distance.
