The galaxy presents a morphology suggestive of an interaction or merger event. Two distinct luminous components are observed, one significantly more concentrated and spheroidal in appearance, and the other more diffuse and elongated. The spheroidal component exhibits a smooth, relatively featureless profile, indicating an older stellar population and potentially less active star formation in the recent past. The elongated component displays a less regular structure, possibly exhibiting tidal features or distortions indicative of gravitational interaction. There is a color variation, with bluer hues at the edges, indicative of active star formation in certain regions. This suggests ongoing or recent tidal interactions may be triggering localized star formation. The overall system appears to be undergoing a dynamic process of merging or interaction, leading to the observed morphological disturbances and potential bursts of star formation.
