The galaxy presents as a slightly elongated, lenticular or early-type spiral system. It is observed at a moderate redshift. The central bulge appears prominent and displays a yellowish hue, potentially indicating an older stellar population. The overall color suggests a higher concentration of stars that are in later stages of evolution. There may be faint arm structures or a disk component, which seem to be viewed close to edge-on, but these features are not sharply defined. The galaxy does not display any obvious signs of a current major merger event, but it appears to exhibit some degree of asymmetry, suggesting a possible minor disturbance or past interaction.
