The object is a spiral galaxy, observed at a redshift indicating a relatively nearby location. The galaxy presents a distinct disk structure, which is not edge-on. Two prominent spiral arms are clearly visible, winding moderately around the galactic center. A weak bar is present in the central region. The bulge appears to be of moderate size, contributing significantly to the overall luminosity of the galaxy, but not dominating it entirely. There is no evidence of a major ongoing merger, though some minor disturbances may be present.
