This galaxy appears to be a spiral galaxy, exhibiting a clear disk structure. The central bulge presents a concentrated, bright yellowish hue, indicating a likely population of older stars. Fainter spiral arms extend outwards from the bulge, displaying a bluer color suggestive of ongoing star formation. The arms appear tightly wound. There is no major disturbance or obvious sign of an ongoing merger. A weak bar is present, subtly elongating the central bulge along its major axis.
