The galaxy presents a smooth, elliptical morphology. Its shape is elongated, appearing more as an "in-between" spheroid rather than perfectly round. The central region is a bright, concentrated bulge that fades gradually into the outer regions. Color gradients indicate a possible change in stellar population and composition from the core to the outskirts. There's a lack of distinct spiral arms or features, giving it a smooth appearance. The galaxy shows no obvious signs of ongoing major merger activity. The color suggests it has a lower ongoing star formation rate.
