The galaxy presents a largely smooth, elliptical morphology, with a high degree of central concentration. The light distribution appears mostly uniform, lacking prominent spiral arm structures or distinct star-forming regions. The galaxy exhibits a notable reddish-yellow hue in its central regions, with a somewhat greenish tint near the edge of the halo, likely suggesting an older stellar population and a moderate amount of ongoing star formation. The overall shape is consistently rounded, with a very slight elongation. There is a possibility of a minor gravitational interaction or disturbance suggested by slight asymmetry in the halo's outer reaches, but this is not a strong indication. Overall, the galaxy appears to be a relatively undisturbed, massive system with a dominant spheroid component.
