The galaxy presents as a roughly elliptical structure, viewed at an angle that indicates it is likely disk-shaped. There is a bright, concentrated central bulge dominating the galaxy's luminosity. The disk component appears relatively smooth and lacks prominent spiral arm structures. The color gradient suggests an older stellar population with a bias towards redder wavelengths. No significant dust lanes or star-forming regions are apparent in this image, indicating a low rate of current star formation. The overall structure suggests a relatively evolved galaxy with a stable morphology. Minor disturbances in its galactic structure cannot be ruled out but are not distinctly visible.
