The galaxy presents as a system of two distinct, yet interacting, components. The primary component exhibits a smooth, rounded morphology, with a bright, concentrated core. The color of the core is distinctly blue, suggesting active star formation. The secondary component appears less defined, with a more diffuse and less concentrated light distribution. It is located in close proximity to the primary component, and there is some evidence of tidal interaction or distortion in the surrounding area. There is a faint trail connecting the two components, which suggests either a recent merger, tidal disruption, or ongoing gravitational interaction. The overall system exhibits a relatively low level of star formation, but the bluer color of the core suggests it is more active than the surrounding regions of the galaxy. The system appears relatively isolated, with no other nearby galaxies in the immediate vicinity. The smoothness of the primary component suggests it could be an elliptical galaxy undergoing interaction with a smaller, irregular galaxy.
