This galaxy exhibits a morphology suggestive of a spiral or disk galaxy, although with some irregularities. The light distribution is not perfectly smooth, and there may be faint spiral arm structures. A possible disturbance is suggested by the galaxy's shape and features. Some of the features could be the result of a minor merger or interaction. It shows a distinct blue hue, particularly in regions that may correspond to spiral arms. The blue color indicates the presence of younger, hotter stars, suggesting ongoing star formation within these regions. The central region shows signs of having more evolved stellar population.
