The galaxy exhibits a spiral morphology, though the spiral arms appear somewhat tightly wound. Two dominant spiral arms are discernible, emanating from the central region. There's a notable central bulge component that comprises a substantial portion of the galaxy's overall luminosity. The galaxy shows a clear disk structure. There are no obvious signs of ongoing major mergers or significant tidal disturbances, though subtle asymmetries might indicate minor interactions. The winding of the spiral arms suggest possible ongoing compression in certain regions. The galaxy is not viewed edge-on, allowing for a clear view of the disk and spiral structure.
