This galaxy appears to be a relatively smooth, elliptical system. It presents a largely featureless profile, lacking prominent spiral arms or dust lanes. The light is centrally concentrated, with a gradual decrease in surface brightness towards the outer regions. The core exhibits a bright, almost stellar-like concentration, which may indicate the presence of an active galactic nucleus or a dense star cluster. The overall shape is nearly circular, showing minimal signs of elongation or asymmetry. There is a hint of color gradient, transitioning from a bluer hue in the central region to a slightly redder tone in the outskirts, suggesting variations in stellar populations or dust content. The lack of significant morphological disturbances suggests it has not undergone a recent major merger event, though subtle distortions could be present upon closer inspection.
