The galaxy presents as a spiral galaxy, observed nearly face-on. A prominent central bulge is visible, exhibiting a yellowish-white hue, indicative of an older stellar population. The spiral arms emanate from this central region, displaying a tightly wound structure with blue regions which suggests active star formation. Some of the spiral arms appear less distinct. A strong central bar structure is observed which spans the galaxy. The disk component exhibits a blue hue. There is no evidence of significant tidal distortions or ongoing major merger events. The galaxy appears to be an isolated system exhibiting ongoing star formation.
