This galaxy exhibits a generally smooth, elliptical morphology with minimal discernible internal structure. The light profile appears centrally concentrated, suggesting a dominant bulge component. The shape is largely round. There is a slight elongation, but the axial ratio is close to unity. The color is relatively uniform across the galaxy, with a slight bluer hue present, indicating the presence of some younger stellar populations. There is no strong evidence of spiral arms or a prominent disk. There is no obvious evidence of a strong interaction or recent merger event that would cause any morphological disturbance.
