The galaxy exhibits a clear spiral structure. Two well-defined spiral arms emanate from the central bulge, winding outwards in a grand design. The arms appear somewhat flocculent, with a mix of brighter knots and more diffuse regions.

The central bulge is prominent and has a moderate size relative to the disk. The bulge exhibits a yellowish color, suggesting an older stellar population.

The disk component displays a bluer hue compared to the bulge, indicative of ongoing star formation. This is also suggested by the patchy nature of the spiral arms, likely caused by differing levels of active star forming regions. There may be the presence of a weak bar structure within the central region. No major signs of strong tidal disturbances or merging activity are observed, but some minor distortion or asymmetry might be present within the outer regions of the spiral arms.
