The galaxy appears to be composed of two distinct, luminous regions in close proximity, potentially indicating an ongoing or recent merger event. The larger, more northern region exhibits a smoother, more diffuse profile. Its color suggests a population of older stars with little ongoing star formation. The southern region appears to have a more concentrated and well-defined core, with a hint of reddish color indicative of more recent star formation or dust obscuration. There appears to be a faint bridge of material connecting these two regions, implying gravitational interaction and mass transfer. The galaxy as a whole exhibits a relatively compact size and lacks any prominent spiral arm structures. The overall morphology points toward a system in transition, possibly evolving from a disturbed state towards a more relaxed elliptical form.
