The galaxy presents as a relatively smooth, elliptical structure. The core region exhibits a concentrated, bright profile, suggesting a significant stellar density. Moving outwards from the core, the galaxy displays a more diffuse halo. There is a hint of a disklike component. The galaxy appears somewhat elongated along one axis, exhibiting an intermediate ellipticity rather than a perfectly circular shape. Faint tidal features or minor disturbances are visible which may imply a recent or ongoing interaction with another galaxy, though these features are not particularly pronounced. The overall color of the galaxy is slightly on the redder side, indicating an older stellar population with relatively little ongoing star formation. 
