The galaxy presents a morphology consistent with a spiral galaxy viewed at a slight angle to face-on. It exhibits a prominent central bulge that appears yellowish in color, indicative of an older stellar population. Fainter, bluer spiral arms extend outwards from the bulge, displaying some patchiness and a flocculent structure, suggesting ongoing star formation activity. The arms appear somewhat tightly wound around the bulge. The overall color gradient suggests a diminishing stellar population from the center to the outer regions. No significant signs of a bar structure are apparent, nor are there any prominent signs of a recent major merger, though some minor disturbances may be present.
