The galaxy presents as a disk-shaped system, seen at an oblique angle. A prominent central bulge is visible, exhibiting a concentrated, yellowish-orange hue, suggestive of an older stellar population. The disk surrounding the bulge displays a bluer color profile, with some clumpy and diffuse areas, potentially indicating ongoing star formation regions. Some slight distortions are evident, particularly on the lower side of the disk, but the overall morphology appears relatively undisturbed, with no strong evidence of recent major merger activity. The structure of the spiral arms is not clearly defined, rather showing a smoother, flocculent texture.
