The galaxy presents as a slightly elongated, relatively compact object.  It appears to be a disk galaxy seen at an oblique angle.  The galaxy exhibits a moderate central bulge, and the overall light distribution appears relatively smooth and centrally concentrated. The disk shows evidence of internal structure but no distinct spiral arms are visible.  Color gradients suggest a somewhat bluer component in the outer regions of the galaxy. It is classified as a field galaxy with evidence of ongoing star formation. A fainter region is visible on the right, which might indicate a minor disturbance.
