The galaxy appears to be a spiral galaxy with a prominent disk structure. The spiral arms are tightly wound around a central bulge. There is evidence of a bar-like feature extending through the core region of the galaxy.

The bulge appears to be of moderate size, neither dwarfing the disk nor being negligible. The spiral arms are well-defined and show some variation in brightness and color, indicating regions of star formation. There appears to be evidence of more than four spiral arms.

There is no obvious sign of major merging activity affecting the overall structure of the galaxy, although there may be minor tidal disturbance. The galaxy displays a generally ordered and symmetrical structure.
