The galaxy presents as a spiral galaxy, exhibiting a distinct disk structure. The disk is not perfectly face-on, showing a slight tilt. Prominent spiral arms are visible, appearing tightly wound around the central bulge. These arms display a blueish hue, potentially indicating regions of active star formation. Two primary spiral arms are discernible. A bar-like structure seems to traverse the central bulge, extending into the inner disk region. The central bulge is moderately sized relative to the disk. Overall, the galaxy displays a morphology consistent with late-type spiral galaxies, with signs of on-going star formation. The galaxy does not appear to be undergoing any major merging events, but there may be some signs of minor disturbance of the shape, though more data would be needed to confirm.
