The galaxy presents a flattened, disk-like morphology, viewed at an oblique angle relative to our line of sight. A central bulge region is observed, though not particularly dominant, exhibiting a moderate concentration of light. Faint indications of spiral arm structure are visible within the disk. A pronounced bar feature appears to extend across the central region of the galaxy. The color distribution suggests a mix of stellar populations, with bluer regions potentially indicative of ongoing star formation and redder regions indicating older stellar populations. There is no evidence of major tidal disturbances, though minor disturbances cannot be ruled out.
