This galaxy exhibits a morphology characteristic of a spiral galaxy, albeit with some indications of a notable bulge component. The spiral arms are visible, although not sharply defined, suggesting a flocculent or grand design structure. The central bulge is relatively prominent, appearing to be of moderate size compared to the disk. There is no strong visual evidence of a bar structure bisecting the central region. Color gradients across the galaxy indicate possible variations in stellar populations, with bluer regions tracing areas of potential star formation activity within the spiral arms. Overall, the galaxy appears largely undisturbed, with no major signs of ongoing merger events or significant tidal interactions. The disk component is not seen perfectly edge on, presenting with an angle that allows some assessment of spiral structure.
