This galaxy exhibits a morphology that is predominantly smooth in appearance. The overall shape is somewhat elliptical, leaning toward a more rounded, but not perfectly circular, form. There is some indication of a disk-like component, which adds to the overall structure.

While the main body of the galaxy is largely undisturbed, there are hints of minor disturbances present. The light profile suggests a central bulge that fades gradually towards the edges. Considering the observed color gradient, there is evidence for ongoing, albeit moderate, star formation activity within the galaxy.

The galaxy shows an intermediate luminosity. The object seems to be at a considerable distance, based on its size and appearance.
