The galaxy presents as a spiral type, exhibiting a well-defined disk structure. Two dominant spiral arms are clearly visible, extending outwards from the central bulge. These arms appear loosely wound, indicating a potentially later-type spiral galaxy. The bulge component is relatively small in comparison to the disk, suggesting a less prominent central mass concentration. Star formation appears active within the spiral arms, as evidenced by the presence of bluer regions and the distribution of light. The overall color of the galaxy indicates a mix of stellar populations, from relatively young blue stars to older, redder stars. There is no strong evidence of a bar structure bisecting the bulge, although a faint, elongated feature may be present within the inner regions of the disk. There is no apparent interaction with any large companion galaxies, though a minor disturbance may be occurring.
