The galaxy presents as a relatively smooth, lenticular or elliptical type. Its morphology is largely featureless, with a centrally concentrated bulge that fades into a diffuse disk. The overall color profile suggests a greater proportion of older stellar populations, exhibiting a redder hue, although there are some blue regions. The galaxy appears elongated, but not particularly flattened. There is no obvious evidence of a recent major merger event, although some minor irregularities or disturbances cannot be ruled out. The galaxy has a moderate apparent size given its redshift.
