The galaxy presents as a spiral with a moderate inclination relative to our line of sight. A central bulge dominates the overall light profile, exhibiting a bright and concentrated core region. The spiral arms are tightly wound and appear somewhat flocculent, displaying a high degree of symmetry. Faint blue regions suggest ongoing star formation. The overall color is slightly redder, potentially indicating a relatively older stellar population. No significant signs of strong tidal interactions or mergers are apparent, although some minor disturbances cannot be ruled out. The galactic disk appears relatively smooth, without prominent dust lanes. There is evidence of a bar structure.
