The galaxy appears as a somewhat smooth, elliptical structure with a discernible central bulge. There are hints of a disk component, but it lacks prominent spiral arms. Coloration suggests some star formation activity, particularly within the disk region, indicated by a slightly bluer hue. The galaxy's overall form does not show obvious signs of major mergers or significant disturbances, although a minor interaction cannot be ruled out based on subtle asymmetries in its outer regions. The galaxy appears relatively compact.
