The galaxy presents as a spiral galaxy with a clearly defined disk structure. Faint spiral arms are visible, emanating from a prominent central bulge. The bulge appears yellowish-white in color, suggesting an older stellar population. The spiral arms exhibit a bluer hue, indicating the presence of younger, hotter stars.

There are suggestions of some dust lanes or patchy structures within the disk. Overall, the galaxy appears relatively face-on, allowing for a good view of its spiral structure. There is evidence of interactions or some type of gravitational disturbance visible at one end of the galaxy. There also appears to be a possible bar present within the galaxy.
