The galaxy presents a generally smooth, rounded morphology, with a high degree of central concentration. The dominant color is yellowish-orange, suggesting an older stellar population and potentially a lack of ongoing star formation. There is a slight extension to one side of the central bulge, possibly indicating a minor tidal disturbance or a faint disk component. The overall structure suggests a classification leaning towards an elliptical galaxy, though subtle features suggest past interaction or a weak disk structure. The galaxy appears relatively isolated.
