The galaxy presents as a barred spiral type, exhibiting a well-defined central bulge and spiral arms. The arms appear flocculent and somewhat tightly wound as they emanate from the prominent central bar. The bar feature itself appears substantial and extends across a significant portion of the galaxy's central region. The color distribution suggests active star formation regions within the spiral arms, contrasted by a possibly older stellar population dominating the bulge region. There's an indication of a slight tilt relative to our line of sight, presenting a somewhat elongated rather than perfectly face-on perspective. The galaxy shows some degree of disturbance or interaction.
