The galaxy presents as a spiral type, with a clear disk-like structure. Distinct spiral arms are visible, demonstrating a relatively tightly wound morphology. A bulge is apparent at the galactic center. The colour distribution indicates a population of young, blue stars present in the spiral arms, contrasted by a slightly redder hue toward the central bulge, possibly indicating an older stellar population. The galaxy appears undisturbed, displaying no significant signs of tidal interactions or recent mergers. Some light obscuration likely exists within the disk, probably due to the presence of dust lanes.
