The galaxy presents a distinct spiral morphology. There is a noticeable central bulge that appears moderately prominent, with a yellowish color suggestive of an older stellar population. Emerging from the bulge are spiral arms, quite distinct, extending outwards. The arms appear somewhat flocculent, exhibiting a mixture of medium and loosely wound structures. There are two dominant spiral arms. These arms contain areas of blue, indicating regions of active star formation. The galaxy is viewed at a moderate inclination, with the disk tilted relative to our line of sight. The overall shape is oval, consistent with a spiral galaxy at this inclination. There are some indications of minor disturbances in the disk, possibly signs of a past interaction or merger event. No strong bar structure is visible at the center.
