The galaxy presents as a spiral type, observed at a slight angle from face-on. It exhibits a prominent central bulge with a bright, concentrated core. Spiral arms are clearly visible, though somewhat tightly wound. The arms display a patchy structure, indicating regions of active star formation. A strong bar-like structure is apparent, extending through the central region. The overall color suggests a mix of stellar populations with a bias towards older, redder stars, although hints of bluer regions can be discerned in the spiral arms. The galaxy appears relatively isolated, with no obvious signs of major mergers, though some minor disturbances in the disk could be present.
