The galaxy appears to be a relatively large system exhibiting a generally smooth morphology. A prominent central bulge is visible, characterized by a high concentration of light. However, there appear to be minor disturbances possibly resulting from a relatively smooth merger, although the disturbances could be internal. There is some light beyond the central region, suggesting either a large disk or an extended halo. The roundness of the galaxy indicates a small amount of angular momentum. There is active star formation occurring within the galaxy, as suggested by the green and red hues.
