The galaxy presents as a centrally concentrated mass, exhibiting a smooth, elliptical morphology. The light is generally distributed evenly, with a gradual falloff in luminosity from the core outwards. There is no discernible spiral structure or any indication of recent or ongoing major mergers or tidal disturbances. The galaxy appears to be relatively compact, with a high degree of symmetry about its center. The galaxy exhibits a noticeable red-shift indicating that it is relatively far away from the observer. The color gradient appears relatively homogenous across the galaxy.
