The object presents as a spiral galaxy, viewed at an oblique angle. Prominent spiral arms are visible, displaying a somewhat flocculent structure. The arms exhibit variations in color, with regions of bluer hues, suggestive of ongoing star formation, interspersed with regions of yellower, redder hues, indicative of older stellar populations and dust. A central bulge is apparent, appearing relatively small to moderate in size and yellowish/whitish color. The spiral arms suggest a moderate winding, neither tightly wound nor particularly loose. There are two main arms with a few smaller ones, for a total of 2. A subtle bar-like structure may be present within the central region. The overall morphology does not indicate a recent major merger event, though some minor disturbances or asymmetries may be present in the outer arms and overall shape.
