The galaxy presents a prominent disk structure, viewed at a significant inclination. Spiral arms are evident, exhibiting a grand design with flocculent characteristics. These arms appear relatively tightly wound, though some show looser extensions. The central bulge is moderately sized, contributing significantly to the overall luminosity. There is no obvious presence of a strong bar structure bisecting the nucleus, nor is there evidence for a dominant bulge. Star formation appears to be ongoing within the spiral arms, contributing to their patchy appearance. The galaxy does not appear to be currently undergoing a major merger, although minor disturbances or interactions cannot be entirely ruled out based on this image.
