The galaxy appears to be a spiral galaxy, presenting an edge-on or nearly edge-on orientation relative to our line of sight. There is a pronounced central bulge, exhibiting a yellowish-orange hue suggestive of an older stellar population. A faint, diffuse disk extends outward from the bulge. The disk displays a bluish tint, hinting at the presence of younger, hotter stars and ongoing star formation. The elongation is quite strong, and it shows a smooth profile. There is a faint hint of disturbed morphology, maybe due to the presence of a satellite galaxy or previous merger event.
