The galaxy presents a primarily disk-like morphology, oriented at a significant inclination relative to the observer's line of sight. The dominant feature is a prominent disk exhibiting well-defined spiral arm structure. These arms are traced by regions of apparent recent star formation, indicated by their bluer color. The winding of the spiral arms appears moderate. A central bulge is present, though not overtly dominant. There is no strong evidence of a bar structure. There may be an interacting galaxy or tidal debris below the main disk.
