The galaxy presents as two distinct components: a concentrated, yellowish core on the left, and an extended, elongated feature of a bluish hue towards the right. The core appears relatively smooth and featureless, suggesting an older stellar population. The elongated component shows signs of irregularity, possibly indicative of active star formation or tidal disturbances. Its morphology suggests a possible spiral arm viewed edge-on, or perhaps a tidal tail resulting from a past interaction. Overall, the galaxy appears to be undergoing some form of interaction or experiencing internal processes that are disrupting its morphology.
