The galaxy presents as a system undergoing a merger. The morphology suggests interaction between two distinct components: a dominant, relatively smooth, spheroidal component, and a fainter, more diffuse component that may exhibit tidal features or signs of disturbance.

The dominant component exhibits a smooth luminosity profile. It displays a slightly elongated shape, suggesting it is not perfectly spherical.

The second component has a lower surface brightness, and appears more diffuse. Its color indicates a region of active star formation, distinct from the older stellar populations of the primary component. The overall morphology indicates potential tidal interactions, such as bridges or tails, linking these components. The system as a whole does not appear to be strongly disturbed; the interaction could represent an early stage merger.
