The galaxy presents as a spiral type, viewed at a considerable angle from face-on. Two primary spiral arms are clearly discernible, exhibiting a loosely wound morphology. The central bulge appears moderately sized and shows a yellowish hue, suggesting an older stellar population. Evidence of active star formation is visible within the spiral arms, indicated by bluer regions. There appears to be an active galactic nucleus that could be creating an emission line. The overall structure hints at a possible interaction or merger event, which is causing tidal disturbances.
