The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing largely rounded in shape with a slight deviation. The central region is significantly brighter and appears yellow, suggesting an older stellar population or dust obscuration. A fainter, more diffuse halo surrounds the core, extending outward. There's no obvious spiral arm structure, bar, or signs of major tidal disruption. There might be a hint of minor asymmetry, but no prominent indication of ongoing mergers or significant interactions.
