The galaxy presents as an interacting system, showing signs of a possible merger in progress. It appears comprised of two distinct components: a primary, more diffuse, yellowish component and a secondary, more compact and bluer component.

The yellowish component exhibits a smooth morphology with a centrally concentrated light profile. Its color suggests an older stellar population likely dominating the light output, implying less active star formation.

The bluer component is smaller and displays a more defined structure. The blue hue indicates the presence of younger, hotter stars and, potentially, regions of active star formation. The juxtaposition of the blue component suggests tidal disturbances or interactions influencing its morphology. The system may eventually coalesce into a single, more homogenous galaxy.
