This galaxy presents as a spiral type, with a moderately defined disk structure exhibiting asymmetrical arm features. The spiral arms appear somewhat flocculent, displaying intermittent concentrations of star formation regions. These regions are characterized by a bluish tint, indicative of younger, hotter stellar populations. Dust lanes are visible, particularly on the near side of the disk, obscuring background light and contributing to the galaxy's overall structured appearance. The central bulge is not sharply defined, showing a gradual increase in luminosity toward the core. A subtle tidal disturbance feature or minor companion is possible.