The object presents a complex morphology, suggestive of an ongoing or recent interaction. At the core of the system, a bright, nearly unresolved component dominates the light profile, possibly indicating a significant bulge or active galactic nucleus. The presence of an adjacent, slightly less luminous component implies a possible merger or tidal interaction. A faint, extended halo surrounds both components, potentially composed of disrupted material from the interaction. The color indices suggest a mixed stellar population, with a predominantly green hue indicating contributions from both young, star-forming regions and older stellar populations. The overall structure departs significantly from a classical elliptical or spiral morphology, showing instead an irregular shape indicative of gravitational disturbance.
