The galaxy appears as a somewhat centrally concentrated object. Its overall structure is relatively smooth, but with subtle irregularities present in the outer regions.

Color gradients suggest variations in stellar populations or dust content. The core region exhibits a slightly bluer hue, which may indicate the presence of younger stars. The outer regions tend towards redder colors, potentially due to older stellar populations or dust obscuration.

There is a slight hint of a disk-like structure, but it is not sharply defined. Possible signs of a minor disturbance, such as a slight asymmetry, can be observed. Overall, the galaxy demonstrates characteristics of a relatively evolved system, with the possibility of ongoing minor interactions.
