The galaxy presents an overall smooth and elliptical morphology. Its shape appears elongated, with a higher probability of being an in-between shape than a completely circular one. The central region exhibits a high surface brightness, appearing significantly brighter and more concentrated than the outer regions. This bright core suggests a substantial concentration of stars and potentially a supermassive black hole at the galaxy's center. Moving outwards from the core, the luminosity gradually decreases. There is some evidence of what may be a faint disk, though its morphology is not clearly defined. There does not appear to be any substantial evidence of spiral arm structures or recent major merger activity.
