The galaxy presents as an elliptical morphology. It exhibits a concentrated central bulge that displays a yellow-orange hue, suggesting an older stellar population and a low rate of ongoing star formation within this region. Emanating outwards from the central bulge, the surrounding regions show a somewhat diffused structure. There may be faint hints of a disk-like structure surrounding the bulge, but it’s not well defined. Overall, the galaxy appears relatively smooth, with no obvious spiral arms or signs of major disturbances or mergers.
