This galaxy exhibits a disk-like structure with prominent spiral arms. The arms appear tightly wound around a central bulge, which seems moderately sized. A bar structure is visible, and is slightly elongated. There is evidence of ongoing star formation within the spiral arms, indicated by blue colors, while the central bulge shows more yellow hues, indicating a population of older stars. The overall disk appears to be at a slight angle to our line of sight, revealing some of the galaxy's three-dimensional structure. There does not appear to be any major tidal distortion or obvious signs of a recent major merger, though there is a slight asymmetry.
