The galaxy presents as a spiral type, observed at an intermediate inclination. It exhibits a prominent, luminous central bulge with an elliptical shape. The bulge is a yellowish-white hue, suggesting a population of older stars. Spiral arms are clearly visible, extending outwards from the central bulge. These arms appear tightly wound. They possess a bluer tint, indicating the presence of younger stellar populations and ongoing star formation. The dust lanes throughout the disk appear somewhat patchy. The overall morphology is not perfectly smooth, but the galaxy does not appear to be undergoing a major merger or significant disturbance.
