The galaxy presents as a spiral type system with a central bulge region and loosely defined spiral arms. The arms exhibit a patchy structure suggesting active star formation regions or dust obscuration. The central bulge appears smooth and concentrated, indicating an older stellar population. The overall color is consistent with a mix of young, blue stars in the arms and older, redder stars in the bulge. There is minor evidence of a possible disturbance, hinting at a past or ongoing interaction with another galaxy. The galaxy is relatively face-on, providing a clear view of its disk structure.
