The galaxy presents as a single, relatively smooth object. Its morphology appears largely elliptical, showing a centrally concentrated brightness profile. The core exhibits a yellowish hue, suggesting an older stellar population. Fainter, bluer light extends outward from the central region, possibly indicating some ongoing, low-level star formation in the outer regions. No strong spiral arm structures or significant dust lanes are apparent. The overall shape suggests a system that is transitioning toward a more spheroidal morphology. There's a hint of a disturbed morphology, but it could also be caused by image quality and distortions.
