The galaxy presents as a spiral with a prominent, moderately sized bulge. The spiral arms are well-defined and display a two-armed structure. The arms appear tightly wound near the bulge and gradually loosen as they extend outwards. Patches of bluer light suggest regions of active star formation within the arms. A slight asymmetry indicates a possible minor disturbance or ongoing interaction. Overall, the galaxy appears to be a relatively undisturbed spiral.
