The galaxy presents as a slightly inclined spiral, though the arm structure is not well-defined, appearing somewhat flocculent. There is a suggestion of a central bulge, elongated along the same axis as the spiral arms, which are tightly wound. The galaxy displays a modest degree of blueness, indicative of recent or ongoing star formation, particularly noticeable in the arms. No significant dust lanes are clearly visible, and the overall appearance suggests a relatively smooth morphology. There is no obvious evidence of a major ongoing merger. There might be some minor tidal disturbances; however, it is difficult to be certain based on the image quality alone.
