The galaxy presents a flocculent spiral structure, exhibiting loosely defined arms emanating from a moderately sized central bulge. The arms display a tightly wound morphology. The galaxy's disk is oriented at a slight inclination relative to our line of sight, with an axial ratio indicating a nearly face-on presentation. The overall color profile suggests a relatively evolved stellar population, with a moderate degree of ongoing star formation evidenced by the subtle blue hues scattered within the arms. No signs of major tidal disturbances or ongoing merger events are immediately apparent, though subtle asymmetries hint at a possible past interaction.
