This appears to be a spiral galaxy, exhibiting a distinct disk-like structure viewed at an angle between face-on and edge-on. The spiral arms are clearly defined and show a moderate degree of winding, appearing relatively tight. There seems to be two main spiral arms that appear to dominate the structure. These arms are punctuated by what could be active star-forming regions, giving them a clumpy appearance. The central bulge is clearly visible, appearing moderately sized in relation to the disk. A bar-like structure seems to be present within the central bulge, though its strength is difficult to determine. The color distribution suggests a mix of stellar populations, with bluer hues concentrated in the spiral arms, indicative of younger, hotter stars, and yellower hues dominating the bulge, potentially indicating an older stellar population. There is no obvious evidence of ongoing major merging activity. The galaxy may be experiencing some minor disturbance.
