The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The light profile suggests a fairly even distribution, lacking prominent spiral arms or distinct structural features. The core exhibits a yellowish-orange hue, possibly indicating an older stellar population. This color gradually fades into a more diffuse, reddish outer region. There is no discernible dust lane or evidence of significant recent star formation observable in this image. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or ongoing mergers, though some faint asymmetry could indicate minor past disturbances. Overall, the galaxy's appearance is consistent with that of a lenticular or early-type spiral galaxy viewed at a significant redshift.
