The galaxy appears to be a relatively smooth, elliptical galaxy, possibly an early-type spiral with a tightly wound disk, as there seems to be no distinct, organized spiral arm structure. It appears to be of intermediate ellipticity, not perfectly spherical, nor highly elongated. The light distribution suggests a strong central bulge or core, with a gradual decrease in luminosity outward from the center. The galaxy shows a blue tinge, which indicates it may host an appreciable amount of younger stars compared to a typical elliptical, or that there's some current star formation occurring within the galaxy. There do not appear to be any signs of major ongoing mergers or significant tidal disturbances. There may be a slight minor disturbance, possibly a smaller galaxy in the process of being accreted.
