The galaxy presents as a spiral morphology, viewed at an oblique angle relative to its disk plane. There is a prominent central bulge with a concentrated, yellowish core region, suggestive of an older stellar population. The spiral arms are relatively tightly wound and exhibit a clumpy structure, indicative of active star formation regions along the arms. These regions display bluer hues, consistent with the presence of younger, hotter stars. The disk appears relatively thin and exhibits subtle color gradients, with the outer regions appearing somewhat bluer than the inner regions. No prominent bar structure is discernible in the image, however, there appears to be a tidal disturbance or a minor merger event, possibly involving a small companion galaxy or some degree of gravitational interaction. There is no indication of a recent major merger event.
