The galaxy presents as a relatively bright, centrally concentrated object. The morphology appears to be largely smooth and elliptical. There is minimal evidence of a disk component or spiral arms. The galaxy exhibits a slight elongation, deviating marginally from a perfectly circular shape. There might be a hint of faint asymmetry or a minor tidal feature, but it is not pronounced. There is some light star formation occurring, but not very significant. The galaxy has a moderate stellar mass. Its redshift indicates that we are observing it as it was roughly 2 billion years ago.
