The galaxy presents as a spiral, likely seen at an oblique angle. The central bulge appears relatively prominent, exhibiting a concentrated, bright yellowish-white hue, suggesting an older stellar population. Fainter blue-ish arms extend outwards, indicating ongoing star formation. The arms are tightly wound. There is no strong evidence of a bar structure. There is also no clear evidence of a major merger. The overall structure seems largely unperturbed, with only possible minor disturbances present.
