The galaxy presents a mostly smooth and concentrated morphology, showing a largely featureless elliptical shape. The central region exhibits a bright, high-intensity luminosity, with a core that appears slightly redder in hue compared to the surrounding regions. The color profile gradually transitions to a bluish tint as the radius increases from the center. There may be very faint hints of spiral arms or a disk, but these are subtle. The overall structure is quite regular, with no significant signs of major disturbances or ongoing mergers. The apparent size is relatively small, suggesting that the galaxy is either intrinsically compact or distant.
