The galaxy appears to be a somewhat elongated, disk-shaped system. Its light profile suggests a relatively smooth, featureless morphology, with the majority of its light concentrated in the central region. The color gradient transitions from a yellowish-orange core to slightly bluer edges, possibly indicating ongoing star formation in the outer regions or differential dust extinction. A slight asymmetry in the outer isophotes might hint at a minor gravitational interaction or past merger event. The overall structure does not exhibit any prominent spiral arms or a strong central bar feature within our resolving power.
