The galaxy appears to be a relatively face-on lenticular or early-type spiral. It presents a generally smooth, elliptical morphology with a high degree of elongation. The color profile suggests a more prominent blue hue towards the galactic center, possibly indicating the presence of a region of star formation. There is a faint suggestion of a disk-like structure, but it is not sharply defined. The galaxy does not exhibit any obvious signs of major tidal disturbances or ongoing merger activity.
