The galaxy presents as a relatively smooth, elliptical-like structure, with a concentrated central bulge. The light distribution appears to be centrally peaked, fading outwards gradually into a diffuse halo. There is a hint of a flattened disk-like component, although this is not sharply defined. The color gradients suggest an older stellar population overall, with the central region appearing more yellow than the outer regions. There are no obvious signs of spiral arms or strong star-forming regions. The galaxy appears undisturbed, lacking any significant tidal features or signs of recent mergers.
