The galaxy exhibits a distinct spiral structure, with two prominent arms emanating from the central region. These arms appear relatively well-defined and exhibit a moderate winding pattern. The central bulge is discernible but appears relatively small in proportion to the overall galactic disk.

The presence of a bar-like structure is strongly suggested, extending across the center of the galaxy. The galaxy disk has visible distinct features, implying significant star formation within.

There is no obvious evidence of a major ongoing merger, however there appears to be some disturbances within the disk suggesting possible minor interaction with another galaxy.
