The galaxy presents a generally smooth, elliptical morphology. A bright, concentrated central bulge dominates the structure, exhibiting a yellowish hue. The surrounding disk appears less defined, showing a faint, greenish-blue tint, possibly indicating regions of ongoing star formation. There is a subtle indication of a disk structure, though it is not sharply defined. The galaxy appears relatively isolated, without any signs of major tidal disturbances or ongoing mergers in the immediate vicinity. The overall color gradient suggests an aging stellar population within the central bulge, contrasted by the bluer, younger stars forming within the disk.
