The galaxy presents a generally smooth, elliptical morphology. The light profile appears centrally concentrated with a gradual decrease in intensity towards the outer regions. The core exhibits a yellowish-orange hue, suggesting an older stellar population. There may be some weak evidence of a disk, however, the galaxy appears mostly spheroidal. The intermediate hues of the galaxy suggest the presence of ongoing, though perhaps reduced, star formation. There's no obvious evidence of a major merger event, though a minor interaction with a smaller object cannot be entirely ruled out. The overall color and morphology suggest a galaxy that is likely massive and relatively evolved, but not entirely quiescent.
