The galaxy presents as a spiral type, exhibiting distinct structural features. It has a bright, moderately sized central bulge that appears to be a yellowish color, indicating an older stellar population. Emanating from the bulge are prominent spiral arms, which are tightly wound and bifurcate along their lengths. These spiral arms appear to be dominated by a younger stellar population with less dust, though they show patchy areas with more dust. There is evidence of a bar-like structure extending from the bulge. It does not exhibit signs of major mergers, though some signs of minor disturbance cannot be excluded. The galaxy's disk is seen face-on.
