The galaxy presents as an edge-on spiral with a prominent central bulge. The bulge exhibits a yellowish-orange hue, suggestive of an older stellar population. A flattened disk extends outward from the bulge, displaying hints of structure, possibly spiral arms, though these are not clearly defined. The disk has a bluer color, potentially indicating ongoing star formation within. The galaxy shows no obvious signs of major mergers, though there could be some minor disturbances within the disk.
