The galaxy exhibits a well-defined spiral structure, with two prominent arms emanating from a central bulge. The arms appear somewhat flocculent in nature, with regions of intense star formation marked by a bluish hue, indicative of the presence of young, hot stars. The central bulge is moderately sized and exhibits a yellowish-white color, suggesting a population of older stars. A faint bar-like structure appears to traverse the central region. The overall winding of the spiral arms is neither tightly wound nor loosely defined, presenting a medium pitch angle. There's a slight indication of tidal disturbances or interactions, however, the galaxy appears mostly unperturbed.
