This galaxy presents as a dual system, potentially in the early stages of interaction or merger. One component exhibits a relatively smooth, elliptical morphology, appearing somewhat rounded in shape. It is characterized by a predominantly red-shifted spectral signature. The second component appears more disk-like and shows evidence of active star formation, indicated by its bluish-green color. This component appears to be significantly inclined with respect to our line of sight. The system displays a subtle, minor disturbance suggesting tidal interactions between the two components may be underway. Overall, the galaxy appears to be a massive system exhibiting a moderate level of star formation.
