The galaxy presents as a generally smooth, centrally concentrated object. There is a somewhat elliptical morphology, with a major axis longer than its minor axis, but the overall shape is still substantially round rather than elongated. The central region exhibits a strong concentration of light, appearing bright yellowish-white. Diffuse light extends outwards from this core region, forming a faint halo around the nucleus. There is a slight color gradient moving outwards from the center. The core has a yellow hue that transitions into a faint greenish color in the outer regions of the galaxy. There is no obvious sign of spiral arm structure or a prominent disk component. No major or minor mergers can be seen, but very slight disturbances cannot be ruled out. The overall appearance of the galaxy suggests a relatively evolved system with a high degree of stellar population homogeneity.
