The galaxy presents as a somewhat elliptical structure, its light exhibiting a smooth gradient from the core to the outer regions. The color profile suggests a significant population of older stars, indicative of a relatively passive star formation history. The galaxy appears largely undisturbed, displaying minimal evidence of recent major mergers or interactions. There might be a very slight asymmetry or irregularity in its overall shape, possibly suggesting minor past interactions, but overall, the morphology aligns with that of an evolved system with a predominantly quiescent stellar population. At an estimated distance corresponding to its observed redshift, this galaxy would be considered a massive system.
