The galaxy exhibits a mostly smooth morphology. It appears generally circular, with a slight elongation. There is a distinct core and halo with a clear difference in color, the core appearing bluer than the halo, which is distinctly green. There is an indication of some minor disruption to the galaxy's structure. While the bulk of the galaxy appears unified, subtle irregularities in the distribution of light suggest a possible interaction or recent merger. The light profile is mostly smooth, but small variations exist. 
