The galaxy presents as a complex system, exhibiting signs of a possible ongoing merger or strong tidal interaction. A bright, relatively circular central component is dominant, displaying a blue-green hue suggesting the presence of young, hot stars and ongoing star formation. This core exhibits a somewhat smooth texture. A secondary, smaller component is visible nearby, appearing more elliptical in shape and possessing a distinct yellow-orange color. The color suggests an older stellar population.

There is an apparent bridge of material faintly connecting these two components. Irregularities in the overall light distribution, coupled with this bridge-like feature, support the hypothesis of gravitational interaction and possible merging activity. A potential tidal tail may be emerging from the system, but more data is needed to confirm. The system displays an irregular morphology, hinting at a dynamic past. Further spectroscopic data and higher resolution imaging are required to fully characterize the stellar populations, kinematics, and the precise nature of the interaction.
