The object presents as a spiral galaxy, exhibiting a notable disk structure. Two prominent spiral arms are discernible, tightly wound around a central bulge. The arms show a granularity suggesting ongoing star formation, with bluer tints indicative of younger stellar populations. The bulge appears moderately sized and yellow. The galaxy is observed nearly face-on. There is no visually compelling evidence of a strong bar structure or any major merger events, though some minor disturbances may be present in the spiral arms.
