The galaxy presents as a spiral galaxy with a bar-like structure traversing its central region. The spiral arms are clearly visible, exhibiting a relatively tightly wound morphology. There is evidence of active star formation along the spiral arms, indicated by the presence of bluer regions. The central bulge appears moderate in size and exhibits a yellowish hue. The galaxy disk is not perfectly edge-on, but displays a noticeable tilt relative to our line of sight. Overall, there are no major signs of an ongoing merger with another galaxy or significant disturbances in its structure, although minor perturbations cannot be ruled out.
