This galaxy presents as a relatively smooth, disk-shaped system. The central bulge appears bright and concentrated, with a somewhat elliptical morphology. The disk component exhibits a blueish hue, suggesting the presence of a younger stellar population and ongoing star formation. There are hints of faint spiral arm structures extending from the bulge, but they are not sharply defined. The overall appearance indicates a galaxy that is neither a pure elliptical nor a fully developed spiral, perhaps an intermediate type or a spiral with less pronounced arms. The galaxy shows no obvious signs of major mergers or significant tidal disturbances in this image, although minor asymmetries or disturbances cannot be entirely ruled out.
