This galaxy presents a moderately inclined disk morphology, exhibiting prominent spiral arm structures. The arms are fairly tightly wound, tracing a clear pattern from the central bulge outwards. The central bulge appears of moderate size, displaying a yellowish hue indicative of an older stellar population. The spiral arms show a bluer color, suggesting ongoing star formation. Patches of redder color are also visible within the arms, possibly indicating regions of dust obscuration or the presence of older, redder stars. The galaxy does not appear to be strongly edge-on. There is no obvious bar structure visible in the image. The overall structure appears relatively undisturbed with no clear signs of a major ongoing merger, although minor disturbances cannot be ruled out at this resolution.
