The galaxy displays a prominent central bulge, appearing moderately sized within the overall structure. Faint spiral arm structures can be discerned extending outwards from the central region. The arms are not sharply defined but rather appear somewhat diffuse. No strong bar feature is apparent within the central region. There is no clear indication of ongoing major mergers, though some minor disturbance or asymmetry in the outer disk is not ruled out. The overall color suggests a mix of stellar populations. 
