The galaxy appears to be undergoing a merger, characterized by two distinct luminous cores. The larger core displays a somewhat elongated morphology, while the smaller core is more circular in appearance. There are faint tidal features, particularly along the edges of the main core, suggesting gravitational interaction and distortion. The color profile indicates the presence of older stellar populations mixed with regions of active star formation. A significant portion of the light emission seems to come from regions rich in ionized gases. The overall structure lacks a defined spiral arm pattern or prominent bulge component, which is consistent with a system disturbed by an ongoing merging event.
