The galaxy presents as a centrally concentrated object, exhibiting a largely smooth morphology with a subtle disk-like component. The shape appears generally rounded, although there is a slight deviation from perfect circularity.  There is a central bright region exhibiting bluer colors, suggesting recent star formation. The outer regions appear redder, indicating an older stellar population. No strong disturbances or signs of merging activity are evident, although a subtle asymmetry might suggest minor interactions in its past. The overall appearance suggests a galaxy of significant mass, experiencing moderate star formation within its core.
