The galaxy presents as a spiral galaxy, characterized by a relatively small, bright central bulge that appears nearly spherical. Two prominent spiral arms emanate from the central region. These arms are loosely wound, exhibiting a flocculent structure with patchy regions of star formation evident as slight irregularities and color variations within the arms. Overall, the disk of the galaxy appears somewhat disturbed, likely due to a minor interaction or internal dynamics. There is no apparent evidence of a strong central bar structure. The galaxy is not presently involved in any major merger activity but may be in the process of a minor disturbance.
