The object presents as an interacting system, seemingly composed of two distinct components in close proximity. The primary component appears diffuse, roughly spherical with a slight elongation. The color profile is complex, with bluer regions concentrated towards one side, possibly indicating active star formation. A secondary, less luminous object is visible nearby, slightly offset. This secondary component is characterized by a more compact appearance and brighter, possibly stellar nucleus. Faint tidal features or disrupted structures appear to extend from the primary component, hinting at gravitational interaction between the two objects. There is no presence of a defined disk structure or spiral arms within either component. The overall morphology suggests an ongoing or recent merger event.
