The galaxy presents as a spiral with a prominent, moderately sized bulge at its center. The spiral arms appear somewhat flocculent and open, suggesting a later type spiral. The arms exhibit hints of resolved star-forming regions, apparent as subtle variations in color and texture. While the disk is viewed at a slight inclination, it is not edge-on, allowing some detail of the spiral structure to be discerned. No significant disturbances or major merger events are readily apparent, but subtle asymmetries could indicate minor gravitational interactions. A slight bar structure may be present, though difficult to discern. The overall color suggests a galaxy with a mix of stellar populations, with a possible dominance of older stars.
