The galaxy appears to be a spiral galaxy viewed at a relatively high inclination. There is a bright central bulge that dominates the galaxy's luminosity. This bulge seems to be a smooth distribution of light.

A faint, flattened disk is visible extending outwards from the bulge. The disk shows some possible signs of spiral arm structure, but this is not very well defined. There is some indication of blue light in these regions that suggests active star formation. The red light is more concentrated closer to the center of the galaxy. The edge of the disk is distorted in some locations, this may imply some tidal interaction with a nearby galaxy.
