This galaxy appears to be a relatively compact object. Morphologically, it appears to be in the midst of a significant interaction. There are two distinct concentrations of light, suggesting either two galactic nuclei or one nucleus undergoing significant disruption. There is some overall smoothness to its light distribution, but a notable fraction appears to be less regular, indicating some disturbance.

The object's is neither distinctly circular nor elongated. The overall color of the galaxy appears slightly blue, suggesting the presence of younger stellar populations, although this could be due to processing artifacts. This supports the interpretation of ongoing star formation activity.
