The galaxy presents as a face-on spiral, exhibiting a notable disk structure. Distinct spiral arms are visible, winding moderately from the central bulge. There appears to be a two-arm structure. The central bulge is moderately prominent. The disk has a slight blue hue, potentially indicative of ongoing star formation within the spiral arms. There is no obvious major merging activity, although there may be some minor asymmetry present in the disk, which is a possible sign of a minor interaction. A faint bar is present across the center of the galaxy. Overall, the galaxy appears as a well-defined spiral with moderate star formation.
