The observed galaxy presents a disk morphology, viewed at a significant inclination. The bulge component appears moderate in size. The arms appear tightly wound around the central bulge region, showing moderate definition. Star formation is likely suppressed. The galaxy's light is relatively homogenous and has weak evidence of a bar structure. The disk is fairly smooth, with no major disturbances or signs of recent merger events. The galaxy displays primarily a two-armed spiral pattern, and the spiral arms appear tightly wound.
