The galaxy exhibits a spiral morphology, presenting with prominent spiral arms. The arms appear tightly wound around a moderately sized bulge. Within the arms there are concentrations of light suggesting active star formation regions. The nucleus presents a yellowish color indicating an older stellar population and a possible supermassive black hole. The galaxy is tilted relative to our line of sight, making it more elliptical in shape. There is no visual evidence of recent major mergers or strong tidal interactions. Faint dust lanes are visible, subtly obscuring light within the arms.
