The galaxy presents as a face-on spiral, exhibiting a centrally concentrated bulge with a moderate amount of light. Two prominent spiral arms emanate from the central region, displaying a medium winding pattern. The color distribution suggests the presence of both older stellar populations in the bulge and ongoing star formation within the spiral arms, implied by a bluish hue within the arms. The galaxy appears undisturbed with no clear signs of major interactions or mergers. It is neither perfectly circular nor strongly elliptical in overall shape.
