The galaxy presents as a relatively smooth, centrally concentrated object, with a generally rounded morphology. There may be subtle internal features or a disk-like structure, but any such structures appear to be faint. The galaxy does not show obvious signs of major mergers or significant disturbances, although a slight asymmetry or minor irregularity cannot be entirely ruled out. There does not appear to be a bright active galactic nucleus. The galaxy exhibits a subtle gradient in color, suggesting a difference in the stellar population or dust content between its inner and outer regions. It exhibits a moderate redshift. The galaxy appears to have a substantial stellar mass. This galaxy appears to have a modest rate of star formation.
