The galaxy presents as a spiral galaxy with a moderately sized bulge. The spiral arms are clearly visible, emanating from the central bulge region. The arms appear somewhat patchy, suggesting ongoing star formation. The galaxy exhibits a disk structure. There are no obvious signs of a strong central bar feature. The overall morphology indicates a relatively undisturbed system, though some mild asymmetry in the spiral arm structure could suggest a minor interaction or internal dynamics. The color gradient indicates a mix of stellar populations, with the bulge likely dominated by older, redder stars and the arms showing bluer regions associated with younger stars.
