The galaxy presents an overall disk-like morphology, though it appears somewhat face-on in orientation. There is evidence of a central bulge component exhibiting a yellowish-orange hue, suggesting an older stellar population is concentrated in this region. Fainter spiral arm structures can be discerned extending outwards from the bulge, although the definition of these arms is not particularly sharp. The arms appear more blueish, indicating the presence of younger, hotter stars potentially within areas of active star formation. The galaxy does not appear significantly disturbed, and there is no obvious presence of any strong merger activity or tidal features.
