This galaxy presents a well-defined spiral structure. The arms are tightly wound around a bright, moderately sized central bulge. The arms exhibit significant star formation activity, indicated by the presence of numerous blueish knots and regions of enhanced luminosity distributed along their length. The overall color suggests a relatively high rate of ongoing star formation. The central bulge appears more yellow, indicative of an older stellar population. No evidence of a strong central bar is apparent, although there may be a small, subtle bar present. The galaxy's morphology appears relatively undisturbed, with no significant signs of a major merger or tidal disruption. The arms exhibit multiple distinct segments, suggesting multiple arms are present.
