The galaxy presents as a disk-shaped structure with a significant bulge. It is inclined to our line of sight, appearing somewhat elongated.

A spiral arm structure is clearly visible, showing a defined pattern. There is evidence of a bar feature, but it doesn't appear to be super prominent.

The central bulge exhibits a strong concentration of light, possibly indicating a relatively dense stellar population. The outer regions of the disk show a bluer hue, consistent with ongoing star formation. Dust lanes are not clearly visible, but may be present. There appears to be some minor disturbance/asymmetry in the disk shape.
