The galaxy presents as a centrally concentrated, smooth object, elongated in shape, without prominent spiral arms or other distinct features. Its color profile suggests a higher concentration of older stellar populations towards the core, with a gradual shift towards bluer hues in the outer regions, potentially indicating ongoing star formation. The overall morphology is suggestive of an elliptical or lenticular galaxy with a relatively high degree of symmetry. There is no obvious evidence of tidal interactions or recent mergers in this particular image. Based on the observed redshift and the extent of the galaxy, it appears to be a moderately sized galaxy at a considerable distance.
