The galaxy presents a clear spiral structure, with two prominent arms emanating from the central region. These arms appear relatively loosely wound and extend outwards a considerable distance. The spiral arms show variations in color and brightness, suggesting differing populations of stars and gas within them. There appears to be a moderate-sized central bulge, contributing to the overall luminosity of the galaxy's core. There is evidence suggesting that the galaxy is potentially undergoing an interaction with a nearby galactic structure. Some signs of disturbance and tidal features imply possible tidal effects. Overall, this is a spiral galaxy with an interesting potential interaction, meriting further observations to characterize its specific properties and dynamics.
