The galaxy presents as a face-on spiral, exhibiting moderate internal structure despite appearing somewhat blurred. Spiral arms are visible, though not sharply defined. Evidence of a central bulge is apparent, with the bulge size appearing moderate relative to the overall galactic disk. A faint bar structure appears to run through the center, though it does not appear to be a strong, well-defined bar. The galaxy's color profile suggests active star formation, although it may be nearing the lower end of the scale, with some redder regions indicating older stellar populations. The overall symmetry of the galaxy is somewhat perturbed, potentially suggesting past or ongoing interactions or minor disturbances. There are two high luminosity areas that make up the majority of the galaxies light.