This galaxy appears to be a relatively smooth, disc-dominated system. It is elliptical in shape, with a high degree of central concentration. A faint, broad disk structure is visible, though it is not sharply defined. There is no prominent spiral arm structure evident, but there is a subtle irregularity in the disk, hinting at a possible minor disturbance. The galaxy's color suggests ongoing star formation, likely at a moderate rate. The presence of a slight color gradient suggests some variation in stellar populations or dust distribution within the galaxy. The system shows no signs of a major merger or tidal features, indicating that it has likely experienced a relatively quiescent evolutionary history.
