The observed galaxy presents a morphology that is largely smooth and concentrated. The light profile suggests a centrally dominant, spheroidal component. There is faint evidence of a disk, the galaxy is mostly round in shape, with some minor deviations from perfect circularity. There are no obvious signs of strong tidal interactions or major merger events. A slight asymmetry or minor disturbance to the galaxy's structure cannot be ruled out. The galaxy's color indicates a relatively old stellar population.
