The galaxy appears to be a relatively smooth, centrally concentrated system. Its morphology is consistent with that of an elliptical galaxy, or possibly a lenticular galaxy seen at a low inclination. There is a noticeable color gradient, with the core region appearing more reddish-yellow, transitioning to a bluer hue in the outer regions. This could indicate a higher concentration of older stars in the galactic center and the presence of younger stellar populations in the outer regions, or a gradient in dust obscuration. There's a slight asymmetry to the outer isophotes, potentially suggesting past minor interactions or ongoing accretion. The galaxy does not show any obvious signs of spiral arms or a prominent disk structure in this image.
