The galaxy presents as a relatively smooth, elliptical-like structure. It appears to be an intermediate roundness, not perfectly spherical but also not highly elongated. The galaxy exhibits a bright central region which fades into a diffuse halo. There's no clear evidence of spiral arms or a well-defined disk structure. Faint disturbances or features may be present suggesting a possible minor interaction or past merger event. The galaxy presents a moderate blue hue, which would be consistent with the light of younger stars.
