The galaxy presents as a spiral galaxy with a moderate bulge. Tightly wound spiral arms extend from the central bulge, exhibiting a flocculent morphology. There is a possible, weak bar structure. Dust lanes are visible within the spiral arms. The galaxy does not appear to be undergoing a major merger, though there may be signs of minor disturbance or a recent merger. The central bulge appears yellowish, indicative of an older stellar population, while the spiral arms show a bluer hue, suggesting ongoing star formation within the disk. The overall form is well-defined.
