The galaxy presents as a well-defined spiral structure, viewed nearly face-on. The spiral arms are tightly wound, emanating from a central bulge, but are otherwise distinct and not flocculent. The galactic bulge appears small relative to the overall disk size, and the nucleus is a bright, concentrated point source of light. The color of the galaxy suggests that it may not have a large population of young, hot stars, or the dust obscures them, with some parts of the disk appearing slightly more blue suggesting more star formation than others. There is no evidence of a strong bar structure. The galaxy appears relatively isolated with no obvious signs of major interactions or mergers. The spiral structure looks quite regular, suggesting it is well ordered. 
