This galaxy presents as a disk-shaped system. The disk exhibits a notable inclination relative to our line of sight. A central bulge component is present but does not dominate the galaxy's overall structure. The disk displays a smooth appearance with evidence of faint spiral arm structures. The galaxy exhibits a bar feature traversing the central region. The observed color gradients suggest a stellar population distribution where bluer, younger stars are present in the disk. The galaxy appears relatively isolated, with no immediately obvious signs of a major ongoing merger event. There are minor disturbances in the galaxy shape that could indicate minor interactions with other galaxies.