The galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical galaxy at a considerable distance. The morphology appears largely featureless, without prominent spiral arms or a distinct disk structure. The light profile seems to be well-behaved, exhibiting a gradual decrease in intensity from the core outwards. It exhibits a moderate redshift, inferring substantial luminosity. The galaxy's color is slightly redder, which may be due to older stellar populations. There appears to be minimal evidence of ongoing major merger activity or significant disturbances to its structure.
