The galaxy presents as a largely smooth, centrally concentrated structure with an ellipsoidal morphology. The core exhibits a high degree of luminosity, appearing bright yellowish-white, potentially indicating a high concentration of older stars or an active galactic nucleus. Moving outward from the core, the luminosity gradually decreases. A faint, diffuse halo is visible extending beyond the main body of the galaxy, particularly along the major axis, suggesting a relatively large spatial extent. There appear to be some subtle irregularities and possible tidal features in the outer regions of the galaxy; this is a faint bluish region at the periphery of the galaxy. The structure is fairly well-defined, but shows mild disturbances, suggesting a possible ongoing or past interaction with another galaxy. There is likely no strong star forming activity in this galaxy.
