The galaxy appears to be a spiral galaxy, viewed approximately face-on. It exhibits a prominent central bulge that appears yellowish-white in color, suggesting an older stellar population within the bulge. The spiral arms are well-defined, showing a predominantly bluish tint, indicative of active star formation regions. Dust lanes are visible within the arms, obscuring some of the starlight. The arms appear to be moderately tightly wound. There is evidence of a bar structure bisecting the bulge. The galaxy shows signs of minor disturbances and potentially a merging event. The overall color profile suggests a significant population of young, hot stars throughout the arms, juxtaposed with a more evolved population in the central bulge.
