The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a high degree of roundness in its overall morphology. There's little to no indication of distinct spiral arm structures or a well-defined disk. The light profile appears to gradually decrease in intensity from the center outwards, without sharp edges or breaks. There are hints of underlying structure, but generally this galaxy has few distinct features. There is no strong evidence of any major tidal disturbances or ongoing merger activity from the image.
