This galaxy appears to be a relatively smooth, elliptical galaxy. Its light is dominated by older stellar populations, suggested by its redder color, with only a small amount of ongoing star formation. The galaxy presents a generally round morphology, exhibiting minimal signs of significant tidal disturbances or ongoing merger activity. There are no strong indications of a pronounced disk structure. The galaxy's overall appearance suggests that it is a mature system, potentially nearing the end of its star-forming lifecycle.
