The galaxy presents as a disk-shaped system viewed nearly edge-on. A central bulge is visible, exhibiting a yellowish hue, possibly indicating an older stellar population. The disk itself appears somewhat diffuse with a bluish tint. The galaxy shows no strong indications of a recent major merger event. There is a slight hint of dust lane absorption along the galactic plane, further supporting the edge-on disk morphology. Based on the color profile, the galaxy is likely undergoing relatively low levels of star formation activity.
