The galaxy exhibits a clear spiral structure, with loosely wound arms emanating from a central bulge. The arms show mottled regions of star formation activity. The bulge appears relatively prominent and concentrated. There is a suggestion of a bar-like structure spanning the central region. The galaxy presents a slightly tilted disk orientation relative to our line of sight. Its overall color suggests an older stellar population and moderate dust content. There is some visual evidence of possible tidal disturbances, implying past interaction with another galaxy or a small ongoing merger.
