The galaxy appears as a centrally concentrated object with a smooth, diffuse morphology. The light distribution suggests a predominantly bulge-dominated system, with a notable lack of distinct spiral arm structures or significant dust lanes. The overall color is indicative of an older stellar population and subdued star formation activity. There may be a subtle extension of the galactic halo or tidal feature extending from the main body of the galaxy. The morphology is generally consistent with an elliptical or S0 type galaxy, residing at a distance implied by its redshift.
