The galaxy presents as a spiral type, characterized by distinct spiral arms emanating from a central bulge. The arms appear relatively tightly wound. The structure is not perfectly face-on, exhibiting a slight inclination relative to our line of sight. The bulge appears moderate in size. The disk is thin and extends beyond the core with visible banding. There may be evidence of some minor disturbances in the morphology; although, a major disturbance is not likely. There does not seem to be a bar present within the galaxy.
