The galaxy presents as a spiral structure with a moderately sized bulge. The spiral arms appear tightly wound and are relatively distinct, displaying a blue hue suggesting ongoing star formation. Two arms are clearly visible. There is an indication of a bar structure crossing the central bulge, though it is not particularly strong or prominent. The overall color suggests a galaxy with active star formation and a relatively high metallicity. There is no obvious evidence of a major merger or tidal disturbance.
