The galaxy presents as a centrally concentrated object with a generally smooth appearance. The core exhibits a yellow-white hue, suggesting an older stellar population. Evidence of tidal disruption in the form of an extended halo exists in the region. The halo's light is more diffuse and slightly redder.

Based on the overall morphology, the galaxy appears to be in the process of merging. There are what appear to be two distinct nuclei within the single object, with one main center and a secondary center. The central concentration appears generally circular, with the primary nucleus. The two nuclei do not appear to be fully coalesced and show signs of significant disruption.
