The galaxy presents as a face-on spiral, exhibiting a bright, concentrated central bulge with a yellow-white hue. The surrounding disk appears less defined, exhibiting a bluer color profile, likely indicative of more recent star formation. The spiral arms are not sharply delineated but are suggested by subtle variations in color and density within the disk. There is some asymmetry in the distribution of light in the outer regions of the disk, potentially indicative of past interactions or mergers, but the overall structure appears relatively undisturbed. No strong tidal features are obviously apparent. The galaxy shows some evidence of ongoing star formation, most prominently in the outer regions of the disk.
