The galaxy presents as a lenticular or early-type spiral galaxy at a redshift indicating a significant distance. Its overall morphology is characterized by a relatively smooth light distribution, suggesting an older stellar population. There is faint evidence of a possible disk structure, but the light is dominated by the central bulge component. The galaxy appears slightly elongated, but not extremely so. There is also some evidence of possible minor disturbance of the light, which may be indicative of interactions with other galaxies. The color profile shows a redder central region, and the outer regions appear slightly bluer.
