The galaxy presents a largely smooth, elliptical morphology. The core region appears bright and concentrated, with a yellowish hue suggestive of an older stellar population. Proceeding outward from the core, the light profile gradually diminishes, forming a diffuse halo around the center. There is little evidence of spiral arm structure or significant dust lanes within the galaxy. The general roundness and lack of discernible features point towards a classification as an elliptical galaxy, potentially an early-type galaxy that has largely ceased active star formation. There is a slight elongation in one direction but is largely round. No prominent tidal features or signs of recent major mergers are visible in this imaging. The outer edges fade smoothly into the background sky, suggesting a well-mixed and dynamically relaxed system.
