The galaxy presents as a generally compact object with an apparent radius of approximately 2 arcseconds. It exhibits a bluish hue, suggesting the presence of a population of relatively young, hot stars. While the galaxy appears largely smooth, a faint, ring-like structure is visible, potentially indicating the remnants of a past interaction or merger. The morphology appears generally undisturbed, though subtle asymmetries hint at minor internal dynamics. The galaxy may be undergoing a period of relative quiescence, based on the observed lack of prominent features. There may be a faint disk component, but the resolution is insufficient to determine detailed spiral arm structure.
