The galaxy presents a morphology that is suggestive of an ongoing merger event. There appear to be two distinct nuclei visible, indicating that what might have been two separate galaxies are in the process of merging into a single system. The primary body of the galaxy exhibits a relatively smooth appearance, however, there is some degree of disturbance. This disturbance is characterized by irregular light distribution and a diffuse envelope surrounding the main body, possibly indicative of tidal interactions. The overall color index appears redder in the galaxy, suggesting a population of older stars and reduced ongoing star formation within the system. The galaxy is relatively compact and of moderate luminosity.
