The galaxy appears as a centrally concentrated, elliptical-like structure. The core is a bright, yellowish hue, possibly indicating an older stellar population. Moving outwards from the core, the light fades gradually into a diffuse, slightly bluer halo. There is no strong evidence of spiral arms or a distinct disk structure, which suggests a relatively smooth and featureless morphology. The overall form is well-rounded. Faint, subtle disturbances might be present in the outer regions, but these are difficult to discern definitively. The galaxy seems relatively isolated, with no prominent signs of ongoing or recent major merger events.
