The galaxy presents as a somewhat face-on spiral, exhibiting a prominent central bulge that appears yellowish-white. The disk structure is discernible but not sharply defined, showing a bluer hue suggestive of ongoing star formation. There is a slight asymmetry in the distribution of light in the disk. The spiral arms are not well-defined and seem somewhat flocculent. Overall, the galaxy appears relatively undisturbed, but the slight asymmetry suggests a potential minor interaction in its recent history.
