The galaxy appears to be undergoing a significant interaction, possibly a merger. There are at least two distinct components visible. The brighter, more compact component exhibits a yellowish-white hue, suggesting an older stellar population, and possesses a relatively smooth morphology. The second, less luminous component appears more diffuse with a bluish tinge, indicative of younger, hotter stars and ongoing star formation. This secondary component is elongated in shape, potentially representing a tidal tail or a distorted disk. There is some evidence of faint tidal features, indicating a disturbance to the overall galactic structure. The galaxy displays signs of active or recent interaction.
