The observed galaxy presents a relatively face-on orientation, revealing a prominent spiral structure. The spiral arms appear tightly wound, emanating from a central bulge region. The bulge exhibits a concentrated luminosity, appearing yellowish-white in color. A small bar structure appears to be present in the center of the bulge. The spiral arms display a bluer hue than the central bulge, indicative of ongoing star formation. Patchy regions of star formation are distributed along the spiral arms. The galaxy exhibits a moderate level of disturbance, suggesting possible past interaction or minor merger event. The arms can be described by having three to four observable arms.
