The galaxy presents as a relatively smooth, elliptical-like structure. The core region exhibits a concentrated luminosity, appearing yellowish, suggestive of an older stellar population. The surrounding regions are less luminous, with a subtle fading towards the outer edges. There is a hint of a disk-like structure, though it is not clearly defined and the galaxy appears primarily spheroidal. There's no clear evidence of spiral arms or significant dust lanes. The morphology is largely undisturbed, indicating it is likely not undergoing a major merger, although there may be minor asymmetry present. Overall, the galaxy appears to be a relatively evolved system.
