The galaxy presents a smooth, elliptical morphology. Its central region exhibits a high concentration of light, appearing as a bright, yellowish core that indicates the presence of an older stellar population. Moving outwards from the core, the light gradually diffuses into a fainter, more reddish halo, suggesting a decrease in stellar density and a possible transition to older, redder stars. There is no evidence of spiral arms or significant dust lanes; the overall structure lacks distinct features, lending it a mostly uniform appearance. There may be a slight elongation, however, the galaxy largely appears rounded. There is no clear evidence of any ongoing merging activity or major disturbances in its morphology, with no obvious tidal tails or distorted structures visible.
