The galaxy presents as a centrally concentrated spheroid, likely an elliptical or S0 type. The core region is bright and appears mostly homogenous with hints of yellow-white light, suggesting an older stellar population. The radial light profile appears smooth, with no distinct features such as spiral arms or a bar visible. The outer regions display a gradual decrease in surface brightness. The overall shape appears moderately elliptical, with a slightly elongated form. There is no strong evidence of ongoing major mergers or tidal disturbances. The color gradients are subtle, indicating a relatively uniform stellar population throughout the galaxy. There is a slight hint of bluer light concentrated in the central regions, perhaps indicative of localized star formation.