The observed galaxy presents a morphology that is somewhat ambiguous, appearing neither purely elliptical nor a well-defined spiral. It presents a relatively smooth appearance, with evidence of a possible disk structure. There is a hint of a slight elongation.

The light emitted is primarily in the blue-green wavelengths, suggestive of a younger stellar population and ongoing star formation. Overall, the galaxy appears to be a mid-sized system. Some features could be suggestive of a galaxy merger in progress.
