The galaxy presents as a spiral galaxy, characterized by a central bulge and well-defined spiral arms. The bulge appears moderate in size, exhibiting a concentrated luminosity. Prominent, flocculent spiral arms emanate from the central region, extending outwards and wrapping around the galaxy's disk. These arms display regions of active star formation. The galaxy's overall disk appears relatively face-on, allowing for clear observation of its spiral structure. A subtle bar-like structure appears to exist through the center of the galaxy. There may be a slight interaction or disturbance occurring in the galaxy. The morphology appears primarily disk-like, with prominent spiral arm features.
