The galaxy presents as a system with two distinct components. The primary component exhibits a smooth, concentrated light profile. It appears largely featureless, lacking any readily discernible spiral arms or bar structures. The shape is somewhere between round and elliptical. A secondary component is nearby, with the suggestion of a disk-like structure, oriented at an angle relative to our line of sight. This component displays a more yellowish hue than the primary, suggesting a potentially older stellar population or a higher dust content. There is evidence of some tidal disturbances. The overall system suggests a possible interaction or merger event is occurring.
