The galaxy presents a complex morphology. The central region is dominated by a bright, concentrated core. A fainter, more diffuse halo surrounds the core, appearing somewhat irregular in shape. There is a suggestion of some form of structure or features within the halo region surrounding the central bulge. The galaxy appears to be relatively compact in size. Some areas are visibly brighter than others, suggesting an irregular distribution of stellar populations or dust. The overall color suggests a mix of young and old stars with likely some dust attenuation. There is a possible indication of a minor interaction or disturbance.
