The galaxy presents as a system composed of two primary components. The dominant component exhibits a smooth, elliptical morphology with a concentrated central brightness profile, suggesting an older stellar population and a lack of significant ongoing star formation. This component is colored yellow/gold, which is consistent with an absence of younger, bluer stars.

The secondary component appears less defined. It is more diffuse in appearance and displays a slightly irregular morphology, possibly indicative of tidal interactions or ongoing mergers. Patches of warmer colors suggest more active star formation regions in this component, although they are not as prominent as would be seen in a young spiral galaxy. This secondary component is positioned somewhat close to the main galaxy.

The overall appearance suggests a galaxy that is either in the process of merging or has recently undergone a merger event. The apparent lack of significant recent star formation activity within the primary galaxy indicates that the system is likely evolving towards a more quiescent state.
