The galaxy presents as a spiral type, exhibiting well-defined spiral arms. The arms display a loosely wound morphology. Two dominant spiral arms are observed. The galactic bulge appears moderate in size. Evidence of a bar structure is present, though not pronounced. No major signs of galactic merging or significant tidal disturbances are apparent, although a minor irregularity may be present. The overall color profile suggests ongoing star formation, with a bluer hue observable within the spiral arms.
