The galaxy presents as a spiral type, observed at an angle tilted somewhat away from face-on. The central bulge is significant, exhibiting a moderate concentration of light, appearing yellowish. Spiral arms emanate from the core, with indications of a somewhat grand design structure. These arms appear relatively patchy, and tracing them precisely is challenging at this resolution. The arms show hints of blue-ish regions, possibly indicative of star formation. Overall, the disk appears somewhat disturbed, possibly due to interactions or internal dynamics. No prominent bar structure is readily apparent. There is no obvious sign of a major merger, but there may be some minor disturbance. Spiral arms appear to be loosely wound.
