The galaxy presents a flattened, disk-like morphology, observed at a near face-on orientation. Prominent spiral arm structures are visible, exhibiting a moderate winding pattern. These arms appear somewhat flocculent, lacking the grand design structure seen in some spiral galaxies.

The central region exhibits a noticeable bulge, though it is relatively small compared to the overall disk size. A faint bar-like structure seems to span across the bulge region. Dust lanes are subtly discernible along the inner edges of the spiral arms, particularly in regions closer to the galactic center.

Color variations are present, with bluer hues dominating the spiral arms suggesting ongoing star formation activity. The central bulge region shows a tendency towards yellower/redder colors, hinting at an older stellar population and a relatively quiescent star formation history. Irregularities in the outer disk may be evidence of minor interactions or disturbances.