The galaxy presents as a disk galaxy with a significant spiral structure. The spiral arms appear prominent and loosely wound, likely with at least two clearly defined arms extending from the central region. The central bulge is moderately sized and exhibits a yellow/white hue, indicative of an older stellar population. Star formation appears evident within the arms, as suggested by blue regions in the arms. A weak bar structure may be present in the central region. There are indications of potential interaction or merging events, evidenced by disturbances in the galaxy's overall shape, and potentially major disturbances. The galaxy is not observed edge-on.
