This galaxy exhibits a primarily smooth morphology, with a suggestion of a disk-like structure. The central bulge is prominent and appears more concentrated with a yellowish hue, possibly indicating an older stellar population. The outer regions of the galaxy present a bluer color, hinting at ongoing or recent star formation within those areas. The galaxy's overall shape is more rounded than elongated, with a slight deviation from perfect circularity. There is no strong evidence of major mergers or significant tidal disturbances affecting its current structure, though minor irregularities or disturbances cannot be ruled out. The galaxy appears to be relatively isolated in its immediate environment.
