The observed galaxy presents as a slightly inclined spiral. It appears to exhibit a prominent central bulge region. From what is visible, the outer disk structures reveal evidence of flocculent spiral arms, with moderate winding. The arms are not sharply defined but rather fragmented, with a possible multiple arm structure. The dust lanes are visible, particularly in the regions where the arms are most discernible. Star forming regions are present, appearing as bright knots within the arms. The overall colour profile appears to be blue, suggesting ongoing star formation within the spiral arms. There is no strong evidence of a bar structure, and the galaxy does not appear to be undergoing any major merging event, although a minor disturbance in the disk could be possible. The bulge is moderate in size and luminosity, appearing relatively smooth compared to the more complex arm structures.
