The galaxy presents as a relatively smooth, elliptical structure. Its overall form is elongated, exhibiting an intermediate ellipticity, somewhere between circular and cigar-shaped. The central region appears significantly brighter and more concentrated than the outer regions. The color distribution suggests a slightly redder central bulge transitioning to bluer hues in the outer disk or halo. The galaxy shows no obvious signs of major mergers or strong tidal disturbances. Some subtle asymmetries or minor disturbances may be present, though the resolution limits a conclusive determination.
