The galaxy presents as a system of two interacting galaxies. One is observed almost face on, appearing relatively smooth and elliptical in shape with a concentrated bright nucleus. The other is located nearby, displaying a disk-like structure viewed at an angle, and features a less defined central bulge. The system appears to be undergoing some disturbance. There are hints of potential tidal tails or distortions in the outer regions, suggesting gravitational interaction between the two galaxies is actively occurring. Color analysis indicates the presence of both older stellar populations, visible through the redder hues, and regions of recent or ongoing star formation as evidenced by the bluer light emitted from certain areas, such as the center of the elliptical galaxy.
