The galaxy presents a largely smooth, elliptical morphology. It appears highly rounded, exhibiting minimal deviation from a circular shape. The galaxy's light profile is dominated by a bright, centrally concentrated bulge, indicative of an older stellar population. Fainter, diffuse light extends outwards from this central region. No distinct spiral arm structure or prominent dust lanes are visible, supporting its classification as an elliptical galaxy. There are no obvious signs of recent or ongoing major merger activity; the galaxy appears relatively undisturbed. There might be the faintest suggestion of an outer halo component. The redshift of the galaxy indicates that the light we are observing has been stretched, as expected from looking at distant objects.
