The galaxy presents a generally elliptical morphology. It appears relatively smooth in texture, lacking prominent spiral arms or distinct dust lanes. The galaxy's color profile is predominantly reddish-yellow, suggesting an older stellar population with a lower rate of ongoing star formation. There are subtle hints of disturbed morphology. The core exhibits a more concentrated light profile, indicating the presence of a central bulge. The galaxy is estimated to be of substantial mass, typical for elliptical galaxies. Its observed redshift indicates a significant distance, and therefore an earlier epoch in the universe. There are minor disturbances that indicate the possibility of a previous or ongoing minor merging event.
