The galaxy presents as a relatively compact, ellipsoidal structure with a smooth, diffuse appearance. It exhibits a dominant central concentration of light, suggesting an older stellar population. There is a noticeable lack of distinct spiral arms or other prominent features commonly associated with disk galaxies. The light distribution appears fairly uniform across the galaxy, with a gentle decline in intensity from the core to the outer edges. The color is somewhat yellow-orange, hinting at a population of evolved stars and low current star formation activity. There are some fainter, less defined regions near the main body, which could suggest very minor tidal features or simply variations in stellar density within the galaxy's halo. The overall morphology indicates a galaxy that has likely undergone significant evolution, possibly through mergers or internal dynamical processes, leading to its smooth and featureless appearance.