The galaxy presents as a spiral type, exhibiting a pronounced disk structure. Spiral arms are discernible, with the majority appearing to be tightly wound around the central bulge. The central bulge comprises a significant portion of the galaxy's overall luminosity and displays a yellowish-white color, potentially indicating an older stellar population. The arms themselves show a bluer tint, suggesting ongoing star formation. The disk appears somewhat inclined relative to our line of sight. The galaxy has a slight flattening, and has a smooth appearance. There is the possibility of a weak bar structure. 
