The galaxy exhibits a disturbed morphology, appearing as a probable interacting system. One component displays a diffuse, bluish glow, suggesting ongoing or recent star formation. The bluer regions indicate the presence of younger, hotter stars. The second component appears yellower with a more concentrated center, potentially representing an older stellar population. Tidal features may be present, but are faint and difficult to resolve. The system's overall shape is irregular, further supporting the interpretation of an ongoing interaction or merger event. The galaxy shows intermediate brightness and moderate apparent size.
