The galaxy appears to be a spiral galaxy, seen at an angle somewhat between face-on and inclined. Its disk exhibits a distinct spiral structure. The spiral arms appear fairly tightly wound around a central bulge. There is evidence of a bar structure bisecting the bulge. The bulge has a moderate size.

The galaxy exhibits a blue hue overall, likely indicating the presence of younger, hotter stars within the spiral arms, especially towards the outer regions of the disk. It appears to be a reasonably bright galaxy, exhibiting a clear central concentration of light in the bulge and a gradual fading towards the edge of the disk. There may be evidence of minor disturbance or interaction.
