This galaxy appears to be undergoing a significant interaction, likely a merger or close encounter, with a secondary component. The primary body exhibits a relatively smooth, somewhat round morphology, suggesting an elliptical or lenticular galaxy. The light distribution within this component is centrally concentrated, with a gradual decrease in intensity towards the outer regions. The color appears yellowish.

Adjacent to the primary galaxy is a distinct bluish component. The color suggests a younger stellar population, indicative of recent or ongoing star formation. This component's morphology is less defined, with a more diffuse appearance. This suggests tidal disruption.

The interaction between these two components appears to be significant, potentially influencing the star formation rate and morphology of both galaxies. Evidence of tidal tails or bridges of stellar material is not definitively apparent. The system as a whole appears to be relatively compact, with the two components in close proximity.
