The galaxy presents as a relatively smooth, elliptical or lenticular structure with a centrally concentrated bulge. Its light is dominated by longer wavelengths, giving it a yellow-orange hue. This color suggests an older stellar population. The overall form is fairly rounded, with minimal visual disturbance to its symmetry, with no clearly defined spiral arms, disk-like structures, or tidal features. There may be some signs of minor disturbances but they are not readily apparent. No distinct dust lanes are visible.
