The galaxy presents a largely smooth, elliptical morphology. It exhibits a bright, concentrated central bulge, which appears to be a yellow-orange hue, suggesting an older stellar population. The galaxy shows a gradual decrease in surface brightness moving outwards from the core, though with some faint extended structure. There appears to be little to no evidence of spiral arms or significant dust lanes. It has a slightly elongated shape, not perfectly spherical, but also not very far from round. There are no obvious signs of recent or ongoing major merger events.
