This galaxy exhibits a clear spiral structure. The spiral arms are prominent and relatively tightly wound around the central bulge. It is likely a grand design spiral. The central bulge appears small compared to the size of the galactic disk. The disk component dominates the overall luminosity of the galaxy, the spiral structure is well-defined and not flocculent. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or strong tidal interactions. A weak bar structure might be present in the central region, but further analysis would be needed to confirm this. The winding of the spiral arms suggest there are two of them, potentially. There are some disturbances indicative of minor interaction. The color suggests recent star formation is occurring.
