The galaxy appears to be a spiral type, viewed at an oblique angle, tending towards edge-on. Evidence of a disk is readily apparent. The spiral arms appear well-defined, with a loose winding pattern, indicating they are not tightly wound around the galactic center. I identify two distinct spiral arms.

The galaxy possesses a central bulge of moderate size, that is not overly prominent. The color of the galaxy appears generally blueish. No major signs of ongoing or recent galaxy merging events are immediately obvious, although subtle disturbances cannot be ruled out at this resolution. There is a subtle feature that may be a weak bar structure spanning across the central bulge.
