The galaxy presents as a somewhat elongated structure, appearing to be a spiral galaxy observed at an angle, possibly a side-on view. Its central bulge appears relatively smooth and concentrated, with a slight color gradient suggesting a population of older stars. Fainter arms can be distinguished; they are poorly defined but discernible, with a slightly bluer tinge, which would suggest ongoing star formation. Overall, the galaxy appears to be in a relatively quiescent state, with moderate star formation activity as hinted by the arm colors and absolute magnitudes. Based on morphology, there may be some minor tidal disturbances, possibly from a past interaction. The color indices indicate it is a relatively luminous and massive galaxy.
