The galaxy presents as a distorted spiral, approximately 4 kiloparsecs in radius. The object exhibits a complex morphology, appearing elongated with an irregular, disturbed structure. A distinct tidal tail is visible on one side. It is likely the result of a gravitational interaction. There is evidence of ongoing star formation indicated by the blueish hue, but is dominant in the central regions. The luminosity profile suggests a high mass. There is another galaxy nearby, suggesting the two may be in a tidal interaction with each other.
