The galaxy presents as a spiral structure with a prominent, yet not overwhelmingly dominant, bulge. The spiral arms are well-defined, extending outwards from the central bulge in a grand design. These arms appear to be loosely wound, displaying a flocculent structure. Star formation appears active within these arms, indicated by the presence of bluer knots and regions. The galaxy exhibits a face-on orientation, allowing for a clear view of its spiral morphology. The bulge presents a reddish hue, suggesting an older stellar population, while the spiral arms have a bluer color, indicating ongoing or recent star formation. There are no obvious signs of a strong bar structure, or major merger activity, though some minor disturbances in the outer arms are visible, suggesting potential minor interactions. There are two arms which start from the central bulge and dominate the structure. There are signs of dust lanes within the spiral arms.