The galaxy presents as a spiral type, with a prominent central bulge. The bulge exhibits a bright, concentrated luminosity. Two spiral arms are discernable, extending from the central bulge. These arms appear loosely wound. The galaxy's overall color profile suggests a mix of older stellar populations, with a hint of ongoing star formation within the spiral arms. There appears to be a slight asymmetry to the galaxy's disk, potentially indicating minor disturbances or interactions.
