The galaxy exhibits a morphology that appears generally smooth. However, there is evidence of features that suggest the presence of a disk-like component or spiral arms. The galaxy has a radial profile that doesn't appear perfectly circular. The shape is in between an elliptical and highly flattened disk, and is not fully round. There appears to be some indication of minor gravitational disturbance or perhaps recent interaction with another galaxy. While a substantial fraction of classifications suggest no interaction, there is some visual evidence of asymmetries or irregularities in the galaxy's structure, indicating a possible merger in the relatively recent past. The light is brightest in the core and decreases monotonically with distance from the center. The relative magnitudes in the g, r, and z bands indicate this galaxy is redder in color.
