The galaxy presents as a face-on spiral, exhibiting a prominent disk structure. Spiral arms are visible, though somewhat indistinct and tightly wound around a central bulge. The bulge appears relatively small and features a yellowish hue, potentially indicative of an older stellar population. The spiral arms display a bluer color, suggesting ongoing star formation. Some irregularity is seen within the disk, but it's difficult to ascertain if this is due to minor disturbances or intrinsic structure without higher resolution imagery. There is no visible indication that this galaxy is currently undergoing a merger or exhibiting signs of a major interaction. The central bar structure, if present, appears to be only weak.
