The galaxy presents as a multi-component system, exhibiting characteristics suggestive of an ongoing or recent interaction or merger. A dominant, centrally located bulge exhibits a smooth, relatively featureless appearance, with a yellow-orange hue indicative of an older stellar population. This bulge appears elongated in shape.

A secondary component, located nearby and partially overlapping the primary bulge, displays a bluer color, potentially signifying the presence of younger stars and ongoing star formation. This blue region appears less structured and more diffuse.

Overall, the galaxy displays a moderate luminosity. Irregularities in the overall shape and brightness distribution support the hypothesis of gravitational disturbance due to tidal interactions or a merger event. Based on the colors and shapes, this system is actively evolving, likely transitioning from a phase of intense star formation toward a more quiescent state.
