This galaxy exhibits a distinct spiral structure, possessing flocculent arms that emerge from a prominent central bulge. The arms appear bifurcated and well-defined, demonstrating a relatively consistent pitch angle. The bulge is of moderate size, showing a concentration of older, yellow-hued stars. A bar structure is apparent across the central region of the galaxy, with the bar appearing strong and well-defined. The spiral arms contain patches of blue, indicating regions of active star formation within the galaxy. Signs of minor disturbance and tidal effects seem to be present in the form of asymmetrical features in the distribution of the outer disk, suggesting it may be interacting or merging with another galaxy.
