The galaxy appears to be a relatively smooth, elliptical galaxy at a redshift of approximately 0.215. It exhibits a nearly circular morphology. The core of the galaxy shows a bright, concentrated region, potentially indicating an active galactic nucleus or a high density of stars. The color profile suggests a predominantly older stellar population, as evidenced by the redder hues, but there's a hint of bluer light emanating from the edges indicating ongoing star formation. There is no readily apparent evidence of major mergers or significant tidal disturbances in its structure.
