The galaxy presents as a slightly inclined disk galaxy. There appears to be a central bulge region, exhibiting a more concentrated and yellowish-orange hue, possibly indicating an older stellar population. The disk component is somewhat elongated, and appears to be less structured, lacking distinct spiral arms. The overall color of the disk is a slightly bluer hue compared to the bulge, with a slightly asymmetrical shape, possibly indicating a minor gravitational interaction or merger event. There are no apparent dust lanes or regions of intense star formation visible within the disk at this resolution. The galaxy is moderately bright, suggesting a substantial stellar mass.
