This galaxy exhibits a prominent spiral structure. Two well-defined spiral arms emanate from a central bulge, displaying a grand design. The arms are loosely wound and extend outwards. The central bulge appears to be of moderate size. The disk is not seen edge-on. Evidence suggests the presence of a weak bar structure within the central region. There are no indications of major mergers or significant disturbances, indicating relative isolation. The spiral arms are traced with star forming regions. The core of the galaxy shows a strong presence of light. 
