The galaxy presents as a face-on spiral, with a centrally located bulge. The spiral arms are loosely wound and somewhat patchy in appearance. Blue and white hues are present in the arms, potentially indicating regions of active star formation. The central bulge exhibits a smoother, more homogenous texture compared to the arms. There is no prominent bar structure visible. The overall morphology suggests a disk galaxy with a moderate level of star formation activity. Indications of possible interactions with other galaxies are minor, if present at all, as the galaxy appears relatively undisturbed. The faintness suggests it's a low-mass galaxy.