The galaxy appears to be a spiral galaxy, observed at a slight inclination to our line of sight. There is evidence of spiral arm structure, though they are not sharply defined. These arms exhibit a somewhat flocculent morphology. The central bulge region is moderately prominent, though not the dominant feature of the galaxy. A hint of a bar structure can be seen in the center. The galaxy exhibits a relatively smooth overall appearance, though some minor tidal disturbances cannot be ruled out. The stellar population appears to be a mix of older and younger stars, with a possible ongoing low level of star formation. The disk of the galaxy extends noticeably beyond the central bulge.
