The galaxy presents as a relatively face-on spiral with a pronounced central bulge. The bulge exhibits a yellowish hue, suggestive of an older stellar population. Spiral arms are clearly delineated, appearing somewhat tightly wound, with a blueish tint indicating the presence of ongoing star formation. The overall structure appears disk-dominated. There is no obvious sign of tidal disturbances or major merger events. The galaxy presents a fairly elliptical shape. Bar structures are not apparent.
