The galaxy appears as a relatively compact, elliptical-like structure. Its overall form is largely smooth and featureless, with a high degree of central concentration. The light distribution is somewhat spherical, showing a gradual decline in brightness from the core to the outer regions. There is a clear color gradient within the galaxy. The central region exhibits a yellowish-red hue, suggesting an older stellar population. Moving outwards, the color shifts slightly towards a bluer tone, possibly indicating the presence of younger stars, although this is less pronounced. There is no apparent evidence of spiral arms, a disk, or any significant disturbances in its structure. The galaxy shows no obvious signs of ongoing mergers or tidal interactions.
