This galaxy exhibits a well-defined spiral structure. Two prominent spiral arms emanate from a bright central bulge. The arms are tightly wound, displaying a smooth, almost flocculent texture. The central bulge appears moderate in size, contributing significantly to the galaxy's overall luminosity. There is evidence of a bar structure within the bulge, oriented roughly along the major axis. The galaxy's disk appears to be oriented at a slight angle relative to our line of sight. No significant signs of tidal disruption or major merger activity are detected. The morphology indicates a relatively undisturbed spiral galaxy with moderate ongoing star formation.
