The galaxy presents a distinct spiral structure, with moderately defined arms emanating from a central bulge. The arms exhibit a patchy distribution of luminosity, suggesting areas of active star formation interspersed with regions of lower stellar density. The bulge appears to be relatively prominent, displaying a smoother and more concentrated distribution of light compared to the arms. A bar-like structure seems to extend through the center of the bulge. The orientation of the galaxy is inclined relative to the line of sight, providing a view that is not quite edge-on, but does not reveal a clear face-on perspective. No signs of major interactions or mergers are readily apparent in the immediate vicinity of the galaxy.
