The galaxy presents as a relatively compact and luminous object. Its morphology appears largely smooth, with a generally elliptical shape. There is a suggestion of a slight elongation, but it is predominantly rounded. The color profile indicates a higher concentration of light in the redder bands, which suggests an older stellar population and/or significant dust obscuration. There is no strong evidence of spiral arms or a prominent disk structure. No signs of ongoing major merger activity are readily apparent, though minor disturbances cannot be ruled out at this resolution. Overall, this galaxy appears to be a fairly massive elliptical galaxy at a significant redshift.
