The galaxy presents as a fairly bright, elliptical-like object with a concentrated central bulge and a diffuse, extended halo. The light from the galaxy appears generally smooth, with a hint of flattening suggesting it may be a disk galaxy. There are no clear spiral arm structures or dust lanes visible. There may be some minor internal disturbance in the disk itself. The color of the central bulge has an orangish-red hue which may indicate an older stellar population.
