The galaxy presents a predominantly smooth morphology, suggesting an elliptical or lenticular type. There is a hint of a disk-like structure, but it is not sharply defined. The object displays a yellowish-orange hue indicative of an older stellar population with reduced ongoing star formation. The shape appears somewhat elongated, deviating slightly from a perfectly spherical form. No prominent spiral arms or significant dust lanes are discernible. It may be undergoing a minor disturbance as a merger is possible. Overall, the galaxy appears to be a relatively massive, evolved system with characteristics of both elliptical and early spiral galaxies.
