The galaxy presents as an interacting system consisting of two distinct components. The primary component exhibits a smooth morphology, suggestive of an elliptical galaxy, with a yellowish hue that indicates an older stellar population and suppressed star formation. This component appears relatively round, with minimal discernible structure within.

The secondary component is characterized by a bluer color, which implies the presence of a younger, hotter stellar population and ongoing star formation. This component is less defined in shape, possibly due to tidal disturbances, and its interaction is causing disruptions. There is some evidence of a tidal arm or bridge connecting the two components, which could explain the recent star formation.

The interaction exhibits some disturbance of this system, though overall it appears that the system is stable. 