The galaxy exhibits a somewhat elongated, elliptical morphology. It presents a relatively smooth, diffuse light distribution, with a bright, concentrated central bulge. The outer regions appear fainter and more diffuse, fading gradually into the background. A disk-like structure is present, though not clearly defined, oriented at an angle relative to our line of sight. Color gradients suggest a possible aging stellar population, with a yellowish core. There are no obvious signs of strong tidal interactions or major mergers. There is a subtle blueish tinge in the outer regions of the disk, hinting at the presence of some younger, star-forming regions.
