The galaxy presents as a spiral galaxy, exhibiting a prominent central bulge. The bulge appears relatively bright, suggesting a significant population of older stars. The disk component displays a defined spiral structure, with two readily discernible arms. These arms appear loosely wound, extending outwards from the central bulge. A faint bar feature can be noted across the core. There are regions of active star formation within the arms. There appears to be a minor tidal disturbance in the morphology. The galaxy is viewed at an angle, presenting a somewhat inclined perspective.
