The galaxy exhibits a clear spiral structure, with prominent arms extending outwards from a central bulge. These arms appear somewhat tightly wound. There is evidence of active star formation within these arms.

The central bulge appears to be moderately sized. A weak bar structure may be present, extending across the bulge region. The overall color profile indicates a mixture of stellar populations. The galaxy does not appear to be strongly interacting or undergoing a major merger. It's disc is viewed at more or less face-on inclination. 
