The galaxy presents as a spiral type, viewed at an intermediate angle. It exhibits a distinct disk with prominent spiral arm structure. The arms appear tightly wound in some regions, but medium to loosely wound overall. Two dominant spiral arms are readily discernible, originating from the central region and extending outwards. A prominent bar structure bisects the central bulge, appearing to be strong and well-defined. The bulge itself seems moderate in size relative to the overall disk. There are suggestions of minor tidal disturbances or interactions, possibly indicating an ongoing or past merger event. Overall, the galaxy presents a complex morphology indicative of ongoing dynamic processes.
