This galaxy exhibits a spiral morphology with distinct, loosely wound arms. The spiral structure appears two-armed, with a possible additional arm fragment present. The arms are slightly flocculent in nature. The galaxy shows a small bulge relative to the disk size. There is no indication of a strong bar feature. Evidence suggests the galaxy is undergoing a merger or experiencing some form of gravitational disturbance, as indicated by irregularities in the spiral arm structure and an asymmetrical light distribution. The central region of the galaxy displays a concentration of light, suggesting a relatively old stellar population. Blue colors are less prominent throughout the arms, suggesting a comparatively low rate of recent star formation.
