The galaxy presents as a spiral with a relatively small but clearly defined central bulge. The spiral arms are tightly wound, exhibiting a somewhat flocculent structure. The galaxy's orientation is close to face-on, allowing for a relatively clear view of the spiral structure, which appears to have two dominant arms. The arms display subtle color variations, possibly indicating regions of active star formation or differences in stellar populations. There appears to be only slight asymmetry, suggesting a relatively undisturbed morphology. There is no apparent bar structure. The galaxy exhibits a central concentration of light that gradually fades into the outer regions. There is a hint of a dust lane within the spiral arms.