The galaxy presents as a spiral type with a distinct, centrally concentrated bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population. Spiral arms are apparent, displaying a somewhat flocculent structure. Patches of blue are observed along the spiral arms, indicative of on-going star formation regions. The disk of the galaxy appears relatively smooth and extended, and the galaxy appears somewhat inclined relative to our line of sight. Some apparent disturbance is present, which suggests a possible minor merger event. The galaxy does not appear to have a strong central bar.
