This galaxy exhibits a spiral morphology, and is estimated to be around 7.7 kiloparsecs in radius. The spiral arms appear well-defined, with a tightly wound structure, and feature a non-negligible quantity of H1 gas. The galaxy is of an intermediate angular size. A prominent central bulge is not observed, with a smaller bulge appearing to be present. Evidence of disturbances is observed, and it is believed that the galaxy may be a major merger. A weak or no bar structure appears to be present. It is believed that the galaxy may feature four or more spiral arms. 