The galaxy presents as a centrally concentrated object, exhibiting a largely smooth morphology. It appears somewhat rounded in shape. There may be subtle features or a possible disk-like structure, but these are not clearly defined. No apparent major mergers or significant disturbances are observed, though there may be indications of minor disturbances in the outer regions. Color gradients suggest a higher concentration of older stellar populations toward the center, with bluer hues slightly more prominent at the periphery, hinting at ongoing or recent star formation in those areas, though at low levels. The overall impression is of a relatively evolved system.
