The galaxy appears to be a relatively luminous, disk-like system, though its disk is viewed at an oblique angle. There is a central bulge with a smooth light distribution. The disk shows only faint, diffuse spiral arm structure. The overall color is moderately red, suggesting an older stellar population. There is an indication of ongoing, low-level star formation within the galaxy. There is a slight asymmetry or disturbance, which might suggest a minor interaction with another galaxy. The galaxy is not perfectly round but has a somewhat elongated shape.
