The galaxy presents as a relatively smooth, centrally concentrated elliptical. The core exhibits a yellowish-white hue, suggesting an older stellar population. Moving outward from the core, the color transitions to a bluer shade, hinting at ongoing, although potentially moderate, star formation within the galaxy. The galaxy appears largely undisturbed, with no strong evidence of tidal features or major mergers. There are some subtle irregularities in the outer regions which indicates possible minor disturbances. The general shape is somewhat rounded, with a slight elongation.
