The galaxy appears to be a relatively smooth, elliptical-like structure. The central region exhibits a concentrated, bright luminosity, appearing yellowish. The outer regions of the galaxy gradually fade out, showing a bluer hue. There is a slight hint of a disk-like structure, but it's not prominently defined. There's no clear evidence of significant ongoing merger activity or major disturbances in its overall shape. The morphology is generally smooth, suggesting an older stellar population.
