This galaxy presents as a late-type spiral galaxy with a complex morphology. The disk appears to be oriented at a significant angle relative to our line of sight. While a bulge component is difficult to discern, there is evidence of tidal features or distortions, suggesting a possible past or ongoing interaction with another galaxy. The integrated light profile indicates a blue color, typical of ongoing star formation, particularly within the arms. The presence of distinct knots and irregularities along the spiral arms is noted and likely indicates regions of enhanced star formation. There is a noticeable disturbance in the overall shape, potentially indicative of a minor merger or a significant internal disruption.
