The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a high degree of central concentration. The core region displays a bright, compact luminosity profile, indicative of a high stellar density. Moving outward from the core, the light gradually diminishes, forming a diffuse halo. The overall shape is mostly round with very little evidence of a disk structure or spiral arms. There are no obvious signs of ongoing major merger activity or significant tidal disturbances; any interactions appear minimal. Color gradients suggest a population of older stars. The outer regions show faint traces of ongoing star formation.
